REE Extraction
REE Extraction
com/science/article/pii/S0360128521000526
Manuscript_e187354a8d030abb495d42de2f79eaa5
2 A review of rare earth elements and yttrium in coal ash: content, modes of
4 Biao Fua, James C. Howerb, Wencai Zhang c, Guangqian Luoa, Hongyun Hua, Hong
5 Yaoa*
a
6 State Key Laboratory of Coal Combustion, School of Energy and Power
b
8 University of Kentucky, Center for Applied Energy Research, 2540 Research
9 Park Drive, Lexington, KY 40511, United States of America and University of Kentucky,
11 America
c
12 Department of Mining and Minerals Engineering, Virginia Polytechnic Institute
14 Contact information
20 Rare earth elements and yttrium (REY) have attracted considerable attention over the
21 last decade because of their vital roles in clean energy, consumer product, national
22 defense and security applications, among other uses. Due to the retention of REY
23 during coal burning, coal combustion ash is considered as potential alternative sources
1
© 2021 published by Elsevier. This manuscript is made available under the Elsevier user license
https://www.elsevier.com/open-access/userlicense/1.0/
24 for REY. Understanding the content, speciation, retention and/or transformation
25 behavior of REY during coal combustion not only expand our knowledge of the
26 combustion behavior of the trace elements in coal, but also provide basis for modeling
27 REY partitioning during coal combustion and for developing economically viable REY
28 recovery technologies. This review makes a critical summary of recent progress in the
29 study of REY in coal ash. The contents and the extraction potentials of REY in coal ash
31 evaluated. Various analytical methods for determining REY bulk contents and
32 speciation, together with the solid sample pretreatment, analytical accuracy and
34 analytical approaches combined the indirect methods (e.g., sequential extraction) shed
35 light on the physical distribution, mineralogy, and the chemical state of REY in coal ash.
36 Three types of REY occurrences in coal ash, including Si-Al glassy association,
37 discrete minerals or compounds, and organic association (bound with unburned carbon)
38 were defined in the review. The glassy association can be further divided into REY
39 minerals closely bound to glass phases and dispersed throughout the glassy structure.
40 REY partitioning in various emission streams, the size distribution, and their
41 enrichment behavior in coal ash were discussed. Thermal behavior and transformation
43 REY, REY phosphates, REY carbonates, clay-bound REY and among others were
45 boiler temperature were proposed: the incorporation of the individual REY phases into
2
46 the glass as inclusions and the diffusion of REY phases throughout Si-Al glass
47 structures in the melting process. Feed coal mineral types, mineral-mineral associations,
48 boiler conditions, and other factors control the retention process. After coal combustion,
49 the speciation of REY in fly ash may be modified by the reactions of REY phases with
51 coal combustion was deeply discussed. Finally, current extraction techniques for REY
52 recovery from coal combustion ash were introduced. Future outlooks and research
54 Keywords: Rare earth elements and yttrium; Coal combustion ash; Partitioning
57
3
58 Contents
59 1. Introduction ........................................................................................................................... 6
60 1.1 Background of rare earth elements in coal ash study and their significance ................... 6
61 1.2 Scope of the review ......................................................................................................... 7
62 2. Nature of REY-rich coal........................................................................................................ 9
63 2.1. Nature of REY ................................................................................................................ 9
64 2.2. Contents of REY in coal and REY rich coal ................................................................ 13
65 2.2.1. Abundance of REY in coals around the world ...................................................... 13
66 2.2.2. REY rich coal in major coal-producing countries ................................................. 15
67 2.3. REY occurrence in coal ................................................................................................ 19
68 2.3.1 Proportions of organic and inorganic associations of REY in coal ........................ 21
69 2.3.2. Size and spatial distribution of REY-bearing particles in coal .............................. 25
70 3. Determination of REY in coal ash....................................................................................... 29
71 3.1. Bulk analysis of REY concentration ............................................................................ 31
72 3.1.1. Sample preparation for ICP-based techniques....................................................... 33
73 3.1.2. Inductively coupled plasma atomic emission spectrometry (ICP-OES) ............... 43
74 3.1.3. Inductively coupled plasma mass spectrometry (ICP-MS) ................................... 45
75 3.1.4. Instrumental neutron activation analysis (INAA).................................................. 49
76 3.1.5. X-ray fluorescence (XRF) analysis ....................................................................... 51
77 3.2. Speciation analysis ....................................................................................................... 58
78 3.2.1. Indirect methods .................................................................................................... 58
79 3.2.2. Direct microanalysis methods ............................................................................... 64
80 3.2.3 Synchrotron-based techniques ................................................................................ 69
81 4. Concentrations and valuation of REY in coal ash ............................................................... 76
82 4.1. REY concentrations in world coal ash ......................................................................... 76
83 4.2. REY contents in coal ash from major coal-producing countries .................................. 79
84 4.2.1. Contents and spatial distribution ........................................................................... 79
85 4.2.2. Critical REY ratios ................................................................................................ 82
86 4.3. Estimation of REY reserves and economic value ........................................................ 84
87 4.3.1. Reserve of REY in coal ash ................................................................................... 84
88 4.3.2. Valuation of REY in coal ash ................................................................................ 86
4
89 5. Speciation of REY in coal ash ............................................................................................. 91
90 5.1. Definition and classification of REY forms in coal ash ............................................... 91
91 5.2. Associations with amorphous glassy materials ............................................................ 92
92 5.3. Associations with discrete minerals or compounds ...................................................... 99
93 5.4. Associations with unburned carbon............................................................................ 103
94 6. Behavior of REY in coal-fired power plants ..................................................................... 109
95 6.1. REY partitioning across the coal-fired power plants.................................................. 109
96 6.1.1 Mass balances of REY in power plants. ............................................................... 110
97 6.1.2. Relative distribution of REY among ash streams ................................................ 113
98 6.2. REY partitioning within ash-collection systems ........................................................ 115
99 6.2.1. Variations in REY distribution pattern within ash-collection systems ................ 115
100 6.2.2. Variations of REY in sized fly ash and implications for REY partitioning trend 118
101 6.3. Speciation transformation mechanisms ...................................................................... 121
102 6.3.1. Physical fragmentation ........................................................................................ 121
103 6.3.2. Phase transformation and chemical reactions ...................................................... 123
104 6.4. Further retention mechanisms by fly ash glass ........................................................... 128
105 6.4.1. Origin and formation ........................................................................................... 129
106 6.4.2. Structure and chemistry ....................................................................................... 135
107 6.4.3. Possible incorporation mechanisms of REY into fly ash glass ........................... 138
108 6.5. Overview of REY partitioning mechanisms in coal-fired power plants..................... 146
109 7. Methods for REY recovery from coal ash ......................................................................... 150
110 7.1. Current REY extraction methods ............................................................................... 150
111 7.2. Physical beneficiation................................................................................................. 150
112 7.3. Hydrometallurgical extraction .................................................................................... 153
113 8. Conclusions ....................................................................................................................... 157
114 9. Problems and future outlooks ............................................................................................ 161
115 Acknowledgements ............................................................................................................... 164
116 References ............................................................................................................................. 165
5
117 1. Introduction
118 1.1 Background of rare earth elements in coal ash study and their significance
119 The story of metals recovery from coal ash (i.e. fly ash and bottom ash) can be
120 traced back to the late 19th century, at which vanadium (V) and silver (Ag) were
121 separated from the Poland coal ash [1]. Late in 20th century much attention has been
122 given to coal combustion residues (mainly ash) as potential sources for valuable
123 elements including gold (Au), germanium (Ge), gallium (Ga), and uranium (U) [2]. By
124 the middle of 20th century, U and Ge have been commercially extracted from coal ash
125 residues in the United Kingdom, Soviet Union, and Japan [3–5]. Coal and its ash even
126 became the main U source for the nuclear applications in the post-World War II period
127 [6,7]. Today, the extraction of Ge from the high-Ge coal-derived ash in China and
128 Russian Far East has been the main sources (more than 50%) for world industry [8,9].
129 In case of rare earth elements (herein REYSc represents the sum of the lanthanides, Y,
130 and Sc; REY, REE+Y; REE, if both Y and Sc are not included), several international
131 agencies and national governments have identified REY, especially the middle and
132 heavy REY as the critical metals because of their special applications in the high-tech
135 conventional rare earth ore deposits in recent years, especially the heavy rare earth
136 elements (HREY), stimulated attempts to exploit alternative sources to meet the
137 ever-increasing demand for REY by modern society [11]. Coal and coal ash containing
138 rare metals have again attracted special attention by a number of countries including the
139 United States [12–17], Europe [18–23], China [24–28], Russia [7,29], India [30,31],
140 South Africa [32], Indonesia [33], and among others to alleviate the REY resource
143 possible sources of REY [7,34]. A number of coals, such as the Kentucky Fire Clay coal
144 in Eastern USA [35,36], southwestern China coal [37–39], and Russian Far East coal
145 [29] have been identified with high REY concentration. For detailed knowledge of
146 REE-rich coal deposits, readers are referred to the review by Seredin and Dai [7], Dai et
147 al. [8], and Zhang et al [40]. To evaluate the coal-related materials as resources for REY,
148 Seredin and Dai [7] proposed the cut-off grade for REY oxides (herein used as REO,
149 sum of La2O3 to Lu2O3 plus Y2O3) in coal ash is 0.1%. Most of REY in coal are
150 inorganic minerals (e.g. REY-phosphates) have high melting, boiling, and thermal
151 decomposition temperature [41], allowing them to be enriched in coal ash after removal
152 of organic matter [42]. The concentration of REO in ash residual after REY-rich coal
154 Moreover, the extraction of REY from coal ash has several advantages over the
155 conventional ores, for example fly ash is readily available waste with typical particle
156 size ranging from 0.1-100 µm, which can avoid mining and milling costs spent in the
157 traditional ores (e.g., carbonatite and ion-adsorbed ores). The recovery of REY from
158 coal ash is also an innovative use of coal fly ash with higher economic value. Besides,
159 coal-derived ash is relatively free of radioactive substances compared to the radioactive
160 elements (Th and U) released with the conventional REE ores utilization [10,44]. In
161 brief, the recovery of REY as well as critical metals from these waste materials, if
162 successful on an industrial scale, can both alleviate the REY depletion crisis worldwide
166 published to characterize and extract REY from coal ash, since the United States
7
167 Department of Energy (US-DOE) initiated several projects for recovering REY from
168 coal combustion byproducts in 2014 [17]. Before the extraction of REY from coal ash,
169 it is important to make clear that (1) the concentration, physical distribution, and
170 chemical speciation of REY in coal ash and (2) how these characteristics are associated
171 with the REY extractability. In coal-fired power plants, how REY partition from coal to
172 fly ash and to which constituents the REY are bound in coal ash (i.e., fly ash and bottom
173 ash or boiler slag) are dependent upon factors such as the feed coal properties, the
174 thermal stability of REE species, boiler conditions (temperature, O2 contents, and other
175 parameters), and configuration of the flue gas purification devices. A final viable
176 scheme for REY recovery from coal ash requires identification of ash fractions that
177 enrich REY which are easily leached at mild conditions. Understanding the fate of REY
178 during coal burning in coal-fired power plants can provide a knowledge basis for
179 modeling REE partitioning behavior and for designing proper extraction processes to
181 The recovery of REY from coal and coal ash is ongoing and will be a hot topic in
182 the foreseeable future. Several review papers are available related to the concentrations,
183 speciation, and genetic origin of REY in coal [6,8,9,17] and the recovery methods of
184 REY from coal and coal byproducts [40,45,46]. However, there is no systematic
185 knowledge on the retention and transformation behavior of REY during coal
186 combustion; and a summary of the contents, distribution, and chemical speciation of
187 REY in coal ash as well as the REY extraction methods is lacking. To better understand
188 the resource base and improve the knowledge about REY in coal ash that can be
189 recovered in the future, this paper serves as a summary review of recent work focusing
190 on the contents, distribution, speciation, and recovery methods of REY in coal ash, with
8
191 special attention to the partitioning behavior of REY during coal combustion. The
192 problems and future outlooks are introduced in each section and the end of the paper.
195 As defined by the International Union of Pure and Applied Chemistry [47], rare
197 of lutetium), plus scandium (Sc, atomic number 21) and yttrium (Y, atomic number 21)
199 [Kr]3d14s2, and REE as [Xe]4fn5dm6s2. The similarity in valence electron (outermost
200 shell) is the reason behind the similarities of physicochemical properties among the 17
201 rare earths. Due to differences in electron structures, such as the number of electrons
202 in 4f orbitals, REY shows different properties and each of them has special
204 developed and used to understand their distinct behavior in different processes, such
205 as in rock geochemical evolution history [43,55–59], mineral processing [60–64], and
206 environmental mobility, etc. [65–71]. For coal-related studies, a classification scheme
207 of rare earth elements has been built by dividing the REY into light REE (La to Sm)
208 and HREE (Eu to Lu), with Y sometimes being included among the HREE [36,72,73].
209 Seredin and Dai [7] proposed a threefold classification that is used to divide the REY
210 into light (LREY; La through Sm), middle (Eu through Dy plus Y), and heavy rare
211 earth elements (Ho through Lu)(Figure 1). The ratio of LREE to HREE (L/H) was
212 used to assess the distribution of REE in coal and coal ash [29]. To further evaluate
9
213 coal as a REY raw materials, a threefold industrial division of REY, i.e., critical (Nd,
214 Eu, Tb, Dy, Y, and Er), uncritical (La, Pr, Sm, and Gd) and excessive (Ce, Ho, Tm, Yb,
215 and Lu) groups is proposed [7,78]. Note that the classification of REY into critical,
216 uncritical, and excessive groups is somewhat subjective and transient, contingent
217 upon the global market demands and the supplies on hand [75]. The price of
218 individual REY fluctuated sharply over the last decade [76–79].
219
220
221 Figure 1. The classification of rare earth elements and yttrium according to their
222 geochemical behavior or market price. (after Seredin and Dai [7] and Hower et al.
223 [17])
224
225 The abundance of REY in natural samples follows the Oddo-Harkins rule, in
226 which elements with even atomic numbers are more abundant than odd-numbered
227 elements [80,81]. This effect can also be reflected in coal and coal fly ash (Fig 2a).
229 shape caused by the Oddo-Harkins effects and to compare the fractionation of REY in
10
230 different processes. Average concentrations of REY in world coal or coal ash [82]
231 have been normalized to chondrites [83], Upper Continental Crust (UCC) [84], North
232 American Shale Composite [85], and Post-Archaean Australian Shale Composite
233 (PAAS) for geochemical and coal combustion studies. The former (i.e., chondrites
236 igneous/metamorphic geochemistry. It is known that coal is derived from the upper
237 earth crusts having similar genetic origins to UCC, and therefore, REY in coal or
238 coal-related materials are commonly normalized to the average REY abundance in
239 UCC. In addition to UCC and chondrites, normalization to shale such as the North
240 American Shale Composite (NASC) [85] has been used in some investigations. In
241 presenting REY data, any of the normalization patterns are acceptable.
242
243
244 Figure 2. Plots showing how REE data are presented. (a) Plots of REE
245 abundances in order of atomic number of rare earths, showing “zig-zag” shape
246 constrained by the Oddo-Harkins rule; Promethium (Pm, atomic number (61) is
11
247 omitted because it is not stable in nature; (b) Plots show how normalization of REE
248 concentration data results in smooth patterns for distribution. The average REE
249 concentrations (parts per million) of the materials shown in the legends represents: 1)
250 Chondrites, data from Boynton [83]; 2) the upper continental crust (UCC), data from
251 Taylor and McLennan [84]; 3) the North American Shale Composite (NASC), data
252 from Gromet et al. [85]; and 4) the world hard coal and coal ash, data from Ketris and
254
255 When normalizing to UCC, three enrichment types of REY can be identified
256 [7,34]: L-type (LREY, LaN/LuN > 1; N indicates a value corrected against a standard
257 distribution, such as the Upper Continental Crust), M-type (LaN/SmN <1, GdN/LuN >
258 1), and H-type (LaN/LuN <1). Besides the enrichment types, the following ratios can
259 be used to decouple Ce, Eu, and Gd from the other REE in the distribution patterns
260 [7,34]:
264 (3).
265 Different distribution patterns and the distinct features of Ce, Eu, and Gd correspond
266 to different processes or origins [34], thus REY are a good tracer which has been
267 widely used in the geochemical and environmental studies [67,86–90]. Other
268 definitions of the REY distribution patterns and REY anomalies (e.g., La and Y
12
269 anomalies) are also proposed [29,36,72,73]; therefore, the reader should be cautious
273 A summary of average REY contents in coal from some coal-producing countries,
274 i.e., China, Columbia, Democratic People’s Republic (DPR) of Korea, North Asia
275 (Siberia, Russia Far East, Mongolia, and Kazakhstan), Turkey, and the United States
276 is shown in Table 1. Among the countries, coals from China contained the most
277 abundant REY, followed by Turkey and other countries. Ketris and Yudovich [82]
278 reported that the average abundance of REY in the world coal was estimated to be
279 68.6 µg g-1, comparable to that of UCC (Fig. 2b). On the basis of data from Ketris and
280 Yudovich [82], Zhang et al. [40] estimated a total of ~ 50 million metric tons of
281 REE reserved in world coal, equating to almost half of the REE reserve of traditional
282 REE-bearing ore deposits. Note that the concentrations of REY significantly vary in
283 different coal deposits and different mines, or even show large variations at a single
284 seam in a single mine [36,91–93]. Rare earth elements in coal are usually at trace
285 level (below 0.1 w.t.%). It is necessary to identify REY-rich coal or enrich REY in
286 coal ash (such to meet the requirement for the industrial extraction [40].
287
13
288 Table 1. A summary of REY concentration in major coal-producing countries or regions around the world.
Columbian coal1 China2 DPR Korea coal3 Turkey coal4 US5 North Asia6
289 Values in μg g-1. 1 From Huang et al. [94]. 2 From Dai et al. [95]. 3 From Hu et al. [96]. 4 From Karayigit et al. [97]. 5 From Finkelman et
290 al. [98]. 6 From Arbuzov et al. [99], and the countries of North Asia in their study refer to Siberia, Russia Far East, Mongolia, and
291 Kazakhstan. Ave: the average concentration, µg g-1; Ra: the range of element content, µg g-1; N: the number of coal samples.
14
292 2.2.2. REY rich coal in major coal-producing countries
293 Coal is arguably one of the most complicated rocks on earth [100] and is a
294 typical geochemical barrier that can enrich many precious metals, such as REY, U, Ge,
295 Ga, V, platinum group elements (PGEs), and among others [6,9]. The increasing
296 demand for REY in recent years has stimulated the exploration of alternative rare
297 earth sources including REE-rich coal deposits around the world. Seredin and Dai et
298 al. [7] proposed the cut-off grade of REY concentration for potential industrial
299 utilization. The cut-off value of REO content is required to be greater than 0.1% in
300 coal ash, or 800-900 µg g-1 in coal ash for coal seams with thickness above five
301 meters. The US-DOE set a criterion in their work for assessing raw coal as REY
302 resources: the total REY content shall be greater than 300 µg g-1 on a whole dry coal
303 basis. As shown in Table 2, coal geologists have so far identified several typical
304 REE-rich coal beds (> 0.1%, ash-basis), such as the Pavlovka coal from Russian Far
305 East [29], the Fire Clay coal from central Appalachian basin of Eastern United States
306 [35,36], and the Fuisui and Heshan coals from Sichuan basin of southwestern China
307 [38]. These coals and their corresponding combustion ashes have been considered as
308 potential REY resources. In some literature, the REY-rich coals are broadly referred
309 as ‘metalliferous coal deposits’ or ‘coal-hosted ore deposits’, which had been
310 accurately defined by Seredin and Finkelman [6] as coals with trace element contents
311 10-times higher than the world average. This term has been gradually accepted and
313
15
314 Table 2. Coal samples extremely enriched in REY (µg g-1) from some coal deposits
Thickness REY
Country Region Deposits Ad % Rank N Reference
-1
(m) µg g
316 Notes. Ad represents ash yield of the coal on dry-basis,%; N is the number of coal samples.
317
318 To date, the study of REY-rich coals in the United States and China, including
320 extraction method [27,107,108] have come a long way in the last decade. The United
321 States Geological Survey systematically investigated the spatial distribution of REY
322 in coals from different US coal basins. All the data has been recorded in the USGS
323 Coal Quality database, known as the COALQUAL database with the latest Version
325 Figure 3, samples with REY contents higher than 1000 µg g-1 (ash basis) are densely
326 distributed in the Appalachian and Black Warrior basins. Other regions, including the
327 Illinois, Forest City, and Arkoma basins, etc., are sporadically distributed with
16
328 REY-rich coals. Based on the data of 5378 coal samples from USGS COALQUAL
329 database, Lin et al. [109] estimated that about 9-13% of the samples in the Unites
330 States are promising coals for REY extraction. Bituminous coals from Central
331 Appalachian region, especially from Eastern Kentucky are probably the best option
333
334 Figure. 3. Coal-hosted REE metallogenic zone across the United States. Black dot
335 represents the sample containing REY greater than 1000 µg g-1 (ash basis). The
336 distribution map of REE-bearing coals was obtained from the web-based
338 (https://ncrdspublic.er.usgs.gov/coalqual/).
339
17
340 Coals from China, especially from southwestern China, contain high
342 and their regional tectonic back-ground, two coal-hosted REE metallogenic zones
343 have been recognized, namely the Erlian-Hailaer REY mineralization belt and the
345 first region is situated in the Erlian basin of northeastern China, where the REY-rich
346 coals are mainly formed in early-middle Jurassic period. The average REY
347 concentration of coal is 397.3 µg g-1 and the maximum value can be up to 1461.2 µg
348 g-1. The second coal-hosted REY metallogenic belt locates in the southwestern of
349 China, including coal deposits from Sichuan province, Chongqing city, Guangxi
350 Province, and Yunnan Province. Dai et al. [34,37–39], Zhuang et al.[112,113], Zhao
351 [110,114], and among others [115–118] have studied the REY origins and distribution
352 in the coals from the REY mineralization belt. Average abundance of REY in this
353 region is estimated to be in the range of 874 µg g-1 to 2497 µg g-1 (ash basis) and have
354 thus been considered as promising coals for REY recovery [37,38,92]. According to
358 Overall, the REY-enriched coals from the US and China have been used as
359 steam coal for power generation for many years [16,28,119–122]; the combustion
360 process can further enrich REY in the ash which is beneficial to the extraction. While
361 a few coal-hosted REE ore deposits have been identified worldwide, the uneven
18
362 distribution of REY in different coals from different regions still require a full
363 investigation of REY distribution before the industrial extraction and utilization.
364 Taking the distribution of REY in China as an example, while the average REY
365 content in Chinese coal (136 µg g-1) is higher than the world coal [95], many coal
366 deposits in China cannot be used as potential raw materials for REY extraction. The
367 North China coal basin is the most important coal producing area for China industry,
368 however, the average content of REY in the northern Chinese coals is estimated to be
369 111.2 µg g-1 [123], much lower than the extraction criterion [7].
370
371
372 Figure. 4. Coal-hosted REE metallogenic zone across China coal basins, revised
374
19
375 2.3. REY occurrence in coal
376 The modes of occurrence of REY in coal are important to anticipate their
377 behavior during coal combustion. REY in coal are closely associated with their
378 geological origins, i.e., detrital inputs from the source rocks by wind and water,
379 mineralized REY-rich fluids, and volcanic ash deposits [8,9,34]. Achieving a detailed
380 knowledge of REY speciation in a coal is difficult because: (1) REY enrichment in
382 REY associations [35] and (2) the concentration of an individual element is
383 commonly less than 100 µg g-1. Broadly, REY in coal can be classified into inorganic
384 and organic matter associations (Figure 5) [7,132]. The inorganic forms are the
385 common REY associations in coal including individual REY-bearing minerals (such
387 crystalline structure of accessory minerals (zircon, apatite, etc.), adsorbed to clay
388 minerals, and dissolved in pore waters in coal [7,133,134]. For organic associations,
389 REY in low-rank coal might be bound with carbon functional groups (e.g. -COOH
390 and OH) or form organometallics [72,91,124]. To model the partitioning behavior of
391 REY during coal combustion, study of REY forms in coal should answer the
392 following questions: (1) what is the ratio of each REY associations (mass balance of
393 REY forms) in REY-rich coal? (2) what is the size range of REY-bearing particles in
394 coal and how does REY-bearing phase distribute in coal matrix? (3) what are the
20
396
REY-bearing
INTRINSIC
organometallic compound
ORGANIC
Side chain functional
ADSORBED groups, -COOH, -OH, -
SH, =NH
REY IN COAL
Adsorbed on existing
ADSORBED
minerals, e.g. clays
INORGANIC
Monazite,xenotime,
DISCRETE MINERALS bastnaesite, kimuraite,
lanthanite, florencite, etc.
397
399
401 Besides REY binding forms, the study of different REY associations and their
402 proportions in coal is important to the prediction of REY speciation in coal ash and
405 techniques. Considering the thermal stability of REY-bearing phase, more attention is
406 given to the distribution ratio of REY in organic matter and inorganic matter in coal.
407 In general, coal minerals are the primary hosts of REY especially in high-rank coals
408 [7,133,135]. A part of REY are considered to be associated with organics in low-rank
409 coals, such as lignite [29,72,127]. The first literature supporting the organic
21
410 occurrences of REY in coal might be from Yershov [128], who favored the organic
411 bonding of Y and Yb in Kizelovsk coal from the former Soviet Union. Seredin and his
412 colleagues [29,129] found that about 50% of REY in the lignite and subbituminous
413 coals in the Russian Far East region can be extracted by 1% NaOH, which are
414 considered to be distributed in the humic matter. The organic association of REY in
415 coal was further reported in various coals from different countries, and confirmed by a
416 series of adsorption experiments (adsorption of REY onto humic and fluvic acids, peat,
418 Since early the 1980s, the U.S. Geological Survey (USGS) investigated the
419 modes of occurrence of REY in coals of various ranks (from lignite to bituminous
421 sequential extraction experiments can rapidly provide the opportunity to quantify the
422 REE occurrences in coal. The results showed that REY in most coals occur in
423 monazite, xenotime, and other phosphate minerals, and less than 10% of the total
424 REY existing in US lignite was associated with organic matter [132]. On the basis of
425 summarizing their previous studies and using the same sequential leaching protocol
426 on another 20 international coal samples, Finkelman et al. [125] concluded that most
427 of LREY (> 90%) in coal occurred in mineral phase and about 25-30% HREY had an
428 organic association (Table 3). Further selective leaching on low-rank coals found that
429 more REY were associated with organics than that of high-rank coals. Lin et al. [124]
430 estimated that 25% REY were associated with organics in the low-ash central
431 Appalachian coals. Based on the organic solvent extraction on seven coals from
22
432 Shanxi, China, Wang et al. [91] suggested that REE in organic matter were probably
434 bound to carbon. Dai et al. [133] also found that aluminosilicates were the primary
435 hosts for REE in bituminous coals from Ningxia Province of China. However, there
436 are still disputes on the distribution of LREE and HREE in different occurrence
437 modes.
23
438
439 Table 3. The quantification of the modes of REY in coal by sequential leaching procedure.
U.S. Kentucky coal Bituminous REY 25% of REE bound with organic matter in coal Lin et al. [134]
Lignite and about 50% of the total REY is bound with humic Serdin and
Russia coal
subbituminous matter Shpirt [129]
24
440 In summary, REY in coals have both inorganic and organic associations, and low
441 ash and low rank coals generally have more organically associated REY than high-ash
443 inorganically-associated REY differ between coal deposits and even with samples
444 from a single coal bed, which are certainly a function of geological settings of coal
445 basins (e.g., source-rock properties, volcanic eruptions, etc.), weathering conditions
446 during peat and coal formation, and depositional environment [7,125]. The share of
447 each REY forms in the balance of the total REY in Table 3 is a general result and can
448 be updated with more studies carrying out in the future. To develop reliable sequential
450 double-checked by leaching pure substance and certified coal standards are strongly
451 suggested.
453 The size and spatial distribution of REY-bearing particles in coal are essential to
454 understanding their partitioning behavior during coal combustion. According to the
455 chemical components and the modes of occurrences as noted above, REY-bearing
25
462 Adsorbed onto clays.
463 The size of these REY-bearing particles can vary from several tens of microns
464 (Figure 6a), to several microns (Figure 6b and 6c), to the submicron to nanometer
465 scale (Figure 6d) [37,39,135]. The size and shape of REY particles are associated
466 with their different origins. In addition to the discrete minerals inherited from the
467 source region (i.e., volcanic ash or peralkaline basement rocks of the coal basin)
468 [36,136–138], a number of SEM-EDS studies have shown that the fine authigenic
470 REE-bearing mineralized solutions, are typical forms for the majority of
471 REY-enriched coals. These fine-grained clastic and authigenic REY minerals usually
473
26
474
475 Figure 6. The REY containing mineral grains in coal. (a) rhabdophane distributed
476 along the bedding planes in the late Permian K1-2b coal from the Huayingshan,
477 Sichuan, southwestern China. Reprinted from [136] with permission from Elsevier (b)
478 REY-bearing carbonate mineral (Ca(Mg)CO3F) in the Late Permian coal from the
479 Heshan Coalfield, southern China. Reprinted from [139] with permission from
480 Elsevier. (c) Ce-, La-, Nd-, Ca-rich phosphate (bright spots) distributed in a kaolinite
481 matrix in Fire Clay coal from Eastern Kentucky. Reprinted from [36] with permission
482 from Elsevier. (d) Mixed monazite and kaolinite grain in the Dean coal, Knox County,
484
27
485 The fine particle size of REE-bearing mineral grains and the low concentration
486 of individual REY in coal make the quantification of the size distribution of REY
487 mineral grains a challenging task. Based on the computer-controlled scanning electron
488 microscopy techniques (CCSEM), a research team from the University of North
489 Dakota found that 97 REE-bearing particles of 3307 particles in a lignite are all less
491 https://edx.netl.doe.gov/dataset/70fc29f0-91d5-4fed-83bb-93fe0d0c0c66/resource/45a
493 are in the size range of 0.4-1.0 μm. The particle size of most of REE-bearing phase in
494 REY-rich coal is considered in the size of < 10 μm and some fractions are even
495 sub-micron particles [140]. This provides important information on predicting size
496 distribution of REY in coal-derived ashes. However, there are several severe
497 limitations to quantify the REY containing minerals in coal via CCSEM technique:
498 Even in the REY rich coal, the lower concentrations of REY, especially the
500 The REY minerals are chosen and identified based on their chemical
502 or particles with different chemistry from those in the mineral data files;
503 Interference peaks in some cases appear in the EDS spectra, requiring
505 Nano-sized REE-bearing minerals might occur in other mineral matrices (such
28
507 In addition to the particle size distribution, spatial distribution of REY-bearing
508 particles within single coal particle is another important parameter affecting REY
509 combustion behavior in coal-fired power plants. REY bound with included minerals
510 within coal char might be subjected to a more reducing and a higher temperature
511 condition than the excluded minerals [141,142]. Therefore, the decomposition and
513 electron microscopy studies revealed that REY-bearing mineral particles seemed to
514 occur in the organic maceral of coal [6,35,100,126,143]. Some of them are dispersed
515 into coal maceral, and a part of REY mineral grains are embedded in other mineral
516 matrix, such as clay minerals and carbonates within a coal particle (Figure 6).
518 CCSEM study as illustrated in the technical report further demonstrated that the
520
522 As shown in Figure 7, methods for analysis of REY in coal ash can be divided into
523 the following categories: (1) methods that measure the total REY concentrations and (2)
524 methods that determine speciation of REY in coal ash. Both the bulk elemental analysis
525 and speciation analysis for REY in coal ash are critical to design cost-effective and
526 environmental-friendly extraction methods. The use of various techniques for trace
527 element analysis has been developed for many years; however, a reliable and accurate
528 determination of REY in coal ash still has some problems. This is mainly because (1)
29
529 the complex matrix of the organic/inorganic constituents in coal ash and potential
530 contamination during sampling, preservation, and pretreatment procedure, all of which
531 make REY determination difficult and complicated; and (2) REY associations in coal
532 ash are usually too fine (also few) to be discerned and are heterogeneously distributed
533 among crystalline minerals, amorphous materials, and unburned carbon [144–147],
534 making the accurate speciation analysis very difficult. Therefore, conventional
535 analytical methods used for quantifying REY contents in various materials, including
537 have limitations, such as high detection limits, low sensitivities, poor accuracy, and
538 time-consuming process. These methods are not suitable for REY determination in
539 complicated coal ash and will not be considered in this review.
540 Previous summary of trace elements (mainly toxic elements) determination in coal
541 and coal ash has been quite extensively made, including reviews and papers by Karr
542 [148], Vouropoulos [149], Huggins [150], Bullock [151], ASTM[152]. Nonetheless,
543 few studies focused on the REY determination in coal-related materials. The following
544 section will review the REY analytical methods in coal ash, based on the available
30
Analysis of
REY in coal
ash
Instrumental X- Mass
Absorption/Emissio Direct methods Indirect methods
ray/γ-ray n spectroscopic Spectroscopic
methods methods methods
TEM/SAED/ µXRF
EDS
µXANES
HRTEM/FF
T/EELS
546
547 Figure 7. Subdivision of REY determination methods for coal ash.
548
551 analyses of lanthanides. In the last two decades, the most common analysis methods
552 of bulk REY in coal ash are inductively coupled plasma mass spectrometry (ICP-MS)
555 234, 237-238, 246-247, 250-253, 258-259, 262, 264, 270, 272, 364-367], followed
557 spectrometry (ICP-OES/AES) [15, 22, 30, 31, 33, 122, 140, 159, 161, 163-164, 173,
558 184-186, 231, 236, 363], instrumental neutron activation analysis (INAA) [32, 98,
559 125, 131, 140, 185-186, 211-213, 357], and X-ray fluorescence (XRF) [20-21, 186,
31
560 215-220]. Other common-used techniques for the trace elements analysis in coal ash,
562 spectrometry (AAS), are difficult for quantitative determination of REY, because the
563 stable compounds forming at the flame zone leads to low atomization efficiency and
565 break-down spectrometry (LIBS) for solid samples, are still under development
566 [153]. Hence, the following text reviewed here will focus on bulk analysis of REY in
568
569
570
573 237-238, 246-247, 250-253, 258-259, 262, 264, 270, 272, 364-367], ICP-OES [15, 22,
574 30, 31, 33, 122, 140, 159, 161, 163-164, 173, 184-186, 231, 236, 363], INAA [32, 98,
575 125, 131, 140, 185-186, 211-213, 357], and XRF [20-21, 186, 215-220] used in REY
576 determination in coal ash, data compiled from the published literature over last thirty
577 years.
32
578
581 sample for ICP-based analysis. The first principle for sample preparation for trace
582 element analysis requires producing samples that are representative of the original
585 or pulverized coal into the high temperature plasma [154–156], the precision and
586 reproducibility for the elemental determination are poor [150]. REY-containing
587 aqueous solutions obtained from solid ash particles by acid digestion and/or alkaline
589 161]. Several sample preparation methods, such as acid dissolution, bomb
590 decomposition, alkaline fusion, and sintering have been widely used in numerous
591 laboratories. Here, a short review of the sample pretreatment methods is made before
592 the review of REY analysis through ICP-based techniques. The pretreatment methods
598 Open acid digestion is commonly used for sample preparation for REY
599 determination in coal ash by the means of ICP-OES/MS (Table 4). Several national
600 standard methods have set up detailed digestion procedure using open acid digestion
601 method, such as American ASTM D 6357-19 [152], Chinese Standard MT/T
602 1014-2006 [162], and ISO 23380. It generally involves weighing certain amounts of
33
603 coal ash (0.1g or more), transferring the sample to an anti-corrosive container (e.g.,
604 Teflon cups), and adding concentrated acid and/or other oxidation reagents at a fixed
605 mixing ratio. Next the digestion vessel is placed on a hot plate with all the acids,
606 especially HF, being nearly completed evaporated. The obtained wet solid (mainly
607 salts) is re-dissolved with dilute HNO3, filtered, and diluted to a certain volume.
609 sulfates, and other mineral or mineraloids, can be dissolved with the acid mixtures.
610 However, some REY-bearing particles (such as zircon) may not be dissolved;
611 therefore, higher digestion temperature (130-150 °C) and longer digestion time (at
612 least 5 h) are required for complete dissolution. Obviously, the main advantages of
613 the open hot-plate digestion method over other pretreatment methods are its
614 simplicity and low cost; however, the drawbacks are also evident, including the high
615 amount of acid consumed, acid mist escape, and longer time for the whole digestion
616 process. For example, 40-ml HF plus aqua regia are consumed by the ASTM D 6357
617 method and a longer time, including the ashing, digestion, evaporation, and
619
34
620 Table 4. A summary of the pretreatment methods for REY determinations by the means of hot plate digestion, microwave-assisted digestion,
Hot plate 130 ℃ for, then evaporated and re-dissolved with ICP-OES [15,159,163,164] 85-115%
Hot plate 130-150 ℃, evaporated; add 1 ml HNO3+20 ml H2O ICP-OES/MS [152] 85-115%
heated at 90-100 ℃
Two-step hot plate re-digestion with 1 HNO3+1 H2O2+5 H2O at ICP-MS [165–167] 89-102%
90-100℃ overnight
High pressure closed vessel digested again with 7ml HF at 90 ℃ for 3h, evaporated and ICP-AES/MS [157,168–171] /
35
50mg+1HF+1HNO3, heated at 190℃ for 24 h, then 6ml HNO3
PTFE-lined stainless-steel bombs ICP-MS [28] 95-105%
(40%) heated at 140℃ for 5h for further digestion
Microwave digestion vaporization at 180 ℃, and re-dissolved with 5 ml HNO3 (50%) at ICP-MS [24,27,158,172] /
180 ℃ for 4h
Microwave digestion 0.1g ash+4 ml aqua regia + 2 ml HF, heated at 180 ℃ for 1 h ICP-MS [161]
Microwave digestion HF+HCl+HNO3, EN 13656 method, EN ISO 17294-2 ICP-MS [166] Close to 100%
Hot plate plus microwave 1 hour on a hotplate, then adding 0.5 ml HF and heated for 15
ICP-OES [173] > 95%
digestion min, and the sample was mixed with 8 ml HCl + 2 ml H2SO4,
36
0.05-0.1 g ash + 0.4 g LiBO2, heated at 1000-1100 ℃ for 20 min,
Alkaline fusion ICP-OES/MS [174] 85-115%
re-dissolved with 30 ml 1 + 9 HNO3
Alkaline fusion-hydrothermal agitated with water at 100-105 ℃ for 6h, the precipitate was
ICP-AES [31] /
treatment mixed with 5% NaOH at 100-105 ℃ for 6h, the final filtered solid
37
622 The closed-vessel digestion method, also known as oxygen-bomb decomposition
623 is widely used in rock dissolution for geochemistry studies. It is based on transferring
624 known amounts of samples and mix acid to a Teflon-lined bomb. Then, the closed
625 vessel is stirred, sealed, and placed in an electric oven at a high temperature (190 °
626 C). After dissolution, it is necessary to drive off the acid (HF) at a certain temperature
627 (e.g., 140 ° C). These procedures can be repeated for achieving a complete
628 dissolution of the solid residual. For REY determination, Querol et al. [170,171]
630 determination in coal and coal fly ash (Table 4). Trace elements are sequentially
632 elements). Taggart et al. [16] proposed a simple closed-vessel method for total REY
633 quantification analysis. Coal ash (34 ± 1 mg) was digested overnight at 90-100 °C
634 with 2-ml each of HNO3 and HF. The acidified sample was then evaporated to dryness
636 recovery of NIST fly ash 1633c was in the range of 89.2-102.4%. The closed
637 PTFE-lined stainless-steel bombs or Parr bombs used for dissolving rocks at high
638 temperature and high pressure are also used for coal ash digestion [28,171,177].
639 Overall, the recoveries of closed-vessel digestion were satisfied by comparing the test
640 value to the certified values of NIST SRMs (Table 4). It can be used for REY analysis
641 in ash samples, and the amount of acid volume and the operation steps could be
642 reduced compared to the open acid-digestion method. However, the whole time for
643 the digestion is long and, thus, the working efficiency would be affected if many ash
644 samples need to be analyzed. In addition, care must be taken to avoid (1) the loss of
645 volatile REY species in the vapor that might escape when the pressure is released and
646 (2) the loss of elements by adsorption on the walls of the bomb.
38
647 A number of laboratories use microwave digestion systems to dissolve coal ash
649 digestion, a known amount (~ 0.1g) of coal ashes plus certain volume of mixed acids
650 are digested in a microwave oven. Next, the mixture is heated to remove the HF and
651 re-dissolved with acids. In comparison to open acid digestion and closed vessel
652 digestion, the microwave digestion can greatly reduce the time and acid volume
653 required for the sample dissolution. As shown in Table 4, the longest duration time
654 for microwave digestion reported in the published literature is within two hours and
655 the total volume of mixed acid is generally below 10 ml. Important operation
656 parameters including digestion time, temperature, pressure, acid types, and the ratio
658 different laboratories. All of these parameters affect the detection of REY by
659 ICP-OES/MS [172,173]. However, detailed pretreatment methods or the data for
660 quality control are not reported in many published studies (see the ‘recovery column’
661 in Table 4). Thus, it is recommended that the accuracy and precision of the analytical
663 with other pretreatment methods, few international or national standards give
664 certified microwave digestion methods for ash digestion. Considering the great
665 advantages of microwave digestion over other pretreatment methods, future efforts
667 Finally, alkaline fusion method is also a potential choice for sample preparation
668 for REY determination. It is based on the fusion of ash samples with alkaline
669 materials (lithium meta-/tetraborate, Na2O2, and among others) at high temperature
670 (450 °C or higher). After cooling down, the homogeneous glassy materials are
671 dissolved with HNO3 or HCl. REY in the resulting solutions will be finally analyzed
39
672 by either ICP-OES or ICP-MS. Among the alkaline fusion methods, lithium
673 meta/tetraborate alkaline sintering has been the most popular methods for preparing
674 a liquid sample for REY quantification. Briefly, coal ash is added to lithium
675 metaborate or borate flux, thoroughly mixed, fused in furnace at 1000-1100 °C,
676 and the resulting solids are re-dissolved in diluted HNO3. This method has been
677 written in the ASTM D4503-08 [174] for trace elements determination (REY not
678 included) in solid waste, and has been further used for REY quantification in coal
679 ash in literature [174]. Besides, Na2O2 alkaline sintering was also used in REY
680 determination in ash samples, as proposed and used by several USGS laboratories
681 [174,181,182]. The fusion temperature (450 °C) required in the digestion is
682 significantly lower than that of lithium metaborate or borate fusion method, but acid
683 concentration for the subsequent re-dissolution is higher (25% HNO3) compared to
684 the ASTM alkaline fusion method (5% HNO3). In addition to Li meta/tetraborate
685 alkaline fusion and sodium peroxide sintering, Mondal et al. [31] used alkali fusion
687 Overall, the due to the encapsulation of REY within aluminonsilicate glass of
688 coal ash (see section 5), the analysis of REY requires reagents that can decompose
689 the glass matrix. In comparison to acid digestion, alkaline fusion is more effective
690 in extracting REY from the matrix. Among the alkaline reagents, Na2O2 and NaOH
691 were the most effective reagents for analysis of REY in coal ashes [167]. Attention
692 should be paid to the high procedural blanks for example the introduction of Ba, Ca,
693 and other interfering elements, since a large volume of flux used in the fusion
694 process could be detrimental to trace analysis of individual rare earth elements. For
40
696 method described by the U.S. Geological Survey, because the use of Zr crucible can
698 To further benefit the readers and researchers in measuring REY contents in coal
699 ash, here the DOE-supported round-robin interlaboratory study (RRIS) was served as
700 a typical example to compare the results (also the pros and cons) of different
703 rare earth elements in coal, coal ash, and other related materials for evaluating the
705 methods REY determination in coal ash (Table 4). Eleven materials including coals of
706 different rank, coal fly ashes, coal-bearing rocks, and mine waste as well as four
707 standard reference materials (SRM NIST 1633c, 1632e, 2780a, and USGS SBC-1)
708 were sent to the laboratories and prepared via three procedures:
714 and hydrofluoric) digestion with heating plus the addition of boric acid to
716 The results indicated that Procedure A and Procedure B are effective for total
717 REY extraction from the ash particles (Table 5), showing acceptable recoveries (±
718 15%) for fly ash reference material (NIST 1633c). In terms of the precision, the
719 reproducibility RSD results showed that both open acid digestion (Procedure A) and
41
721 REY that compared with NAA values with lower RSDs (< 5%); and Procedure A
722 performed slightly better than Procedure B because the introduction of alkali
723 reagents into the solution may result in matrix interferences, which should be
724 reduced by diluting the digestion solution prior to ICP-MS analysis. Procedure C, i.e.,
725 the mixed acid digestion with heat plus the addition of boric acid showed the worst
726 mean recoveries (62-96%) and repeatability (RSD > 5%). It is suggested that both of
727 the acid digestion (without boric acid) and the alkaline fusion methods can be
728 effective in REY determination. In addition to these two procedures, any other
729 pretreatment methods can be used before providing appropriate validation with
731 Table 5. The REY recovery rates from NIST 1633 c by using different pretreatment
732 methods.
739 spectrometry (ICP-AES) has been widely used in analysis of REY in coal and coal
741 ICP torch as an excitation source can produce a very high-temperature plasma
742 (7000-10,000 K). Solutions containing REY for analysis are pumped into the
743 nebulizer and sprayed as aerosols into the hot plasma, where it can easily atomize and
744 ionizes the refractory REY. The excited rare earth species naturally emit their unique
745 radiation, which is then detected by the spectrometer. Modern ICP-OES can
748 direct current arc spectrometry or alternating current spark spectrometry : (i) the high
749 temperature (above 7000 K) and electron density (1014-1016 cm-3) of the plasma can
750 destroy almost every species in the sample, minimizing the chemical interferences; (ii)
751 low background emission and chemical interferences; (iii) good accuracy and
752 precision; (iv) wide linear response range; and (v) reasonable costs compared to other
755 significantly when approaching the limits of detection (LOD). To reach an accuracy in
756 the range of 2%, the minimum concentration of the analyte should at least be
757 100-times the LOD. The LOD of the method are sample and matrix dependent, and
758 for lanthanides it is usually in the range of 0.1-100 µg L-1. Usually, the concentration
759 of individual rare earth elements in coal ash is below 100 µg g-1 and a part of REY is
43
760 at sub-µg g-1 level. Thus, quantification of trace amounts of REY in digestion
761 solutions, especially for most HREY (Tb and Ho to Lu) in coal ash is difficult by
762 ICP-OES technique. Readers should be cautioned to the data listed references in
763 Table 4, where most of the ash samples have extremely high total REY contents (>
765 The most important source of instrumental inaccuracy in ICP-OES is the spectral
766 inferences derived from the plasma. The interferences are likely to occur in the
767 analysis of trace REY in coal ash having complex chemical compositions. Especially,
768 the concentrations of Fe, Ca, K, Na, Ti, and Ba in coal ash are several orders of
769 magnitude higher than the REY contents, which may result in the total or partial
770 overlap of analyte (REY) with the interfering species’ lines [187]. Eze. et al. [186]
771 carried out a comparative study of REY determination in coal fly ash using INAA,
772 ICP-OES, XRF, and ICP-MS. Based on analysis of the NIST standard coal fly ash
773 1633b and a South African fly ash, the authors found that REY contents in coal ash
774 determined by ICP-OES are much lower than those by INAA and ICP-MS (Table 6).
775 This is probably caused by the spectra interference or problems occurring in sample
777 analytical line and use software for spectra recognition are important to avoid the
778 inferences in REY analysis. In addition, the ion/cation-exchange separation used for
781
782 Table 6. A comparison of REY concentrations in a South African coal fly ash
783 determined by INAA, ICP-OES, LA-ICP-MS, and XRF. Unit: μg g-1. Data from Eze
786 Note. Conc: the concentration of REY determined by various methods, μg g-1. D.L.:
787 The minimum detection limit, μg g-1. n.d.: not detected. not detected
788
791 determination in coal ash. Just as the ICP source can improve the precision and
792 accuracy of the emission spectroscopy, the same source creates similar improvements
794 shows several advantages: (i) lower detection limits (at ppt level); (ii) wider linear
795 response ranges (up to nine orders of magnitude); (iii) much faster in simultaneous
796 determining multi-elements; (iv) simpler spectra that can avoid matrix separation.
797 Overall, ICP-MS is a better choice for REY determination in coal ash than that of
798 ICP-OES, but the high costs would limit its use in some laboratories.
45
799 To obtain accurate and reliable data, several shortcomings of ICP-MS should be
800 considered including the mass spectral interferences and its intolerance to high
801 contents of dissolved solids (matrix effects) in solutions. For REY analysis, the
802 spectral interferences may arise from the formation of oxide and hydroxide ions in the
803 ICP segment. Table 7 summarizes potential spectral inferences species on REY ions
804 in ICP-MS system. As shown in Table 7, the formation of REE oxide ions (REEO+)
805 especially the occurrence of LREEO+ (with higher ionization energy) that maybe
806 generated from the high-temperature plasma can interfere with the determination of
143
807 the HREE, such as NdO+ on 160
Gd+, 144
SmO+ on 160
Gd+, and 143
NdO+ on 159
Tb+.
808 Fortunately, the yield of REO+ to RE+ is only a few thousandths or lower; and
809 therefore, interferences of LREEO+ on HREE can be neglected due to the lower
810 concentrations of individual REY (at ~ µg g-1 level) in coal ash. However, as Si-rich
811 materials, the determination of Sc in coal ash by ICP-MS may be plagued by spectral
812 interferences from the ash matrix constituents such as Si and Ca, Li and B if using
813 lithium metaborate or borate flux as fusion reagents to digest the ash samples [190]. Li
814 et al. [377] reported that the interferences of B and Ca on Sc analysis are negligible
815 when the B and Ca content is below 100 and 200 µg mL-1 in the final solution for
817 high-resolution ICP-MS [376], algebraic corrections [377], and collision/reaction cell
818 technique [190] during the determination of Sc in siliceous rocks by ICP-MS can be
135
820 Ba-bearing polyatomic ions on Eu isotopes, namely the interference of BaO+ on
46
151
821 Eu+ as well as 137
BaO+ on 153
Eu+ is another problem which must be eliminated if
822 the ash contains high Ba contents [198,199]. Yan et al. [172] used an AG50W-x8
823 cation resin to separate Ba species from the acid digestion solution of coal fly ash
824 samples. Precision and accuracy of their procedure have been demonstrated by repeat
826 coal and fly ash samples. The authors also proposed a ratio of Ba/Eu (1000) as basis
827 for evaluation of the interference of Ba on Eu. If Ba/Eu > 1000, then Ba in coal fly ash
828 can greatly interfere with Eu determination, and measures should be taken to diminish
830
831 Table 7. The potential spectral inferences in REY determination by ICP-MS. After
species te
73
89
Y+ Ge16O+ 154
Gd+ 154
Sm+, 138Ba16O+ 164
Er+ 164
Dy+, 148
Nd16O+,
148
Sm16O+
123
139
La+ Sb16O+ 155
Gd+ 139
La16O+, 138Ba16O1H+ 166
Er+ 150
Nd16O+, 150Sm16O+
124
140
Ce+ Sn16O+, 156
Gd+ 140
Ce16O+ 167
Er+ 151
Eu16O+
124
Te16O+
142
142
Ce+ Nd+, 126Te16O+ 157
Gd+ 141
Pr16O+ 168
Er+ 152
Sm16O+
125
141
Pr+ Te16O+ 158
Gd+ 142
Ce16O+, 142Nd16O+ 170
Er+ 170
Yb+, 154Gd16O+, 154Sm16O
142
142
Nd+ Ce+, 126Te16O+ 160
Gd+ 160
Dy+,144Nd16O+,144Sm 169
Tm 153
Eu16O+
47
16
O+ +
144
144
Nd+ Sm+ 159
Tb+ 143
Nd16O+ 170
Yb+ 170
Er+,154Gd16O+, 154Sm16O
130
146
Nd+ Te16O+ 160
Dy+ 160
Gd+,144Nd16O+,144Sm 171
Yb+ 155
Gd16O+
16
O+
148
148
Nd+ Sm+ 161
Dy+ 145
Nd16O+ 172
Yb+ 156
Gd16O+
150
150
Nd+ Sm+, 162
Dy+ 146
Nd16O+ 173
Yb+ 157
Gd16O+
134
Ba16O+
144
144
Sm+ Nd+ 163
Dy+ 147
Sm16O+ 174
Yb+ 158
Gd16O+
133
149
Sm+ Cs16O+ 164
Dy+ 164
Er+, 148
Nd16O+, 176
Yb+ 176
Lu+,176Hf+,160Gd16O+,160D
148
Sm16O+ y16O+
150
150
Sm+ Nd+, 134Ba16O+ 165
Ho+ 149
Sm16O+ 175
Lu+ 159
Tb16O+
136
152
Sm+ Ba16O+ 151
Eu+ 135
Ba16O+ 176
Lu+ 176
Yb+,176Hf+,160Gd16O+,160D
y16O+
154
154
Sm+ Gd+ 153
Eu+ 137
Ba16O+ 45
Sc+ 7
Li38Ar+,10B35Cl+,
28
Si16O1H+,29Si16O+,
44
Ca1H+,13C16O16O+,
12
C16O16O1H+
833
835 (SF-ICP-MS) in high resolution mode maybe an effective way to reduce the
837 spectrometry (Q-ICP-MS). Thompson et al. [200] carried out a comparative analysis
48
838 of REE in a series of coal-based wastes by Q-ICP-MS and SF-ICP-MS. As revealed,
839 Q-ICP-MS can handle most of geological materials, including coal ash for the
840 determination of REY; whilst, for ash samples containing large amounts of Ba (Ba/Eu >
841 1000), SF-ICP-MS may be suitable to accurately determine all REY (especially Eu).
842 Other methods that have been used to overcome the spectral interferences for
843 environmental samples and geological matrices, including: (1) measure bivalent ions
845 parameters (ICP power, carrier gas flow rate, among others) [205–208], and apply
846 de-solvation techniques [204,209]. These methods could be potential solutions to the
847 accurate analysis of REY in coal fly ash. In addition, both matrix effects and spectral
848 interferences for ICP-MS greatly depend on the sample introduction techniques
849 employed. The pneumatic nebulization for sample introduction brings larger amount
850 of liquids (H2O), which is a main source for generating REEO+ in the ICP source.
851 Ultrasonic nebulization and electro-thermal vaporization (ETV) are alternatives to the
852 solution sample introduction system for ICP-MS. Zhang et al. [190] developed an
855 modifier to promote REY vaporization, solid coal fly ash sample (< 325 mesh) was
856 directly introduced into the ETV system, vaporized in a graphite furnace, and was
857 carried into ICP torch for ionization. Their results revealed that the spectral
858 interferences of matrix elements including Al, Fe, Si, Na, K, Ca, Mg, and Ba on REE
49
860 3.1.4. Instrumental neutron activation analysis (INAA)
862 trace elements (including rare earth elements) in coal and coal ash. The working
863 principal of INAA was built upon the nuclear reactions, where the half-life of
864 radioactive isotopes and the γ-ray energy of each elements are unique and can be used
866 involves: (1) activation process, involving irradiation of the stable isotopes of one
867 element in the sample by thermal neutrons, (2) decay process, involving emission of
868 different types of ionizing radiations during the decay of the radioactive isotopes, and
869 (3) detection of the radiation, such as the β-radiation, γ-radiation, and sometimes
870 determine the decay rate of the radioactive nuclei. Accordingly, the overall test time
871 for INAA analysis requires several weeks, much longer than other instruments [198].
872 This is one of main drawbacks of INAA analysis. Besides, the use of INAA have
874 interferences of major elements in the samples, and high costs of operation [198]; and
875 (2) it cannot analyze the full suite of REY, because the low γ-ray energies for
876 detecting Er and Tm, low sensitivity to neutrons activated from Ho and Y, and no
878 The major advantages of INAA are also obvious: (1) it is a non-destructive
879 analysis technique, material remains intact; (2) sample preparation is very simple, i.e.,
880 drying and weighing mg of test samples without chemical treatment (e.g., dissolution);
881 (3) it allows simultaneous analysis of ~40 radionuclides; (4) a very sensitive
50
882 technique can determine elements at µg g-1 and sub-µg g-1 concentrations. Therefore,
883 INAA has been used for the development and certification of reference materials at
884 national organizations, such as the National Institute of Standards and Technology
885 (NIST).
886 INAA has been widely used to detect trace elements (including rare earth
887 elements) in coal-related materials [150]. For REY determination in coal ash, Tu et al.
888 [212] determined eight rare earth elements (La, Ce, Nd, Eu, Tb, Dy, Yb, and Sc) in a
889 Chinese coal fly ash by the means of INAA using NIST SRMs 1632a as
890 multi-element standards. In their study [212], the procedure in the INAA analysis
891 involved both short and long irradiations with thermal neutron flux (24 h), the decay
892 of the radionuclides (3 weeks), and the measurement of the gamma-ray by a Ge (Le)
169 182
893 detector (4 h). Besides, the γ-ray lines of Yb overlap with Ta at 179.5 keV and
160
894 Tb with 131Ba at 215.8 keV. Thus, INAA cannot be used in routine analysis for most
895 laboratories with such a long measurement period accompanying high costs and long
896 time. Nevertheless, due to its high sensitivity and ability of multi-elemental and
897 non-destructive analysis, INAA has been used as one of the principal reference
898 methods to determine REY in coal ash [32,186,213]. For example, in the
899 DOE-supported REE characterization projects [140], to evaluate the precision and
900 accuracy of the ICP-based REE determination methods, one laboratory applied INAA
901 as the reference method. As illustrated in Table 6, INAA had the best performance in
902 determining REE in coal ash with average REE recovery approaching 100%. Wagner
51
903 et al. [32] gained comparable values of six REEs (Sc, La, Ce, Eu, Sm, and Tb) in five
904 South African coal fly ash samples analyzed by INAA to that of ICP-MS.
907 REY in the solid ash. It is usually used for analysis of major elements in geological
908 and environmental materials [214]. Some researchers, for examples, Kuhn et al. [215]
909 and Prather et al.[216] tried to extend this technique to trace elements analysis in coal.
910 The main advantages of XRF are: (1) in situ analysis of elements without sample
911 preparation, such ashing, milling, pelletization, or digestion; and thus, the overall
912 measurement time is shorter and less expensive relative to other instrumental
913 techniques; (2) simultaneous analysis of both major and minor components; (3)
914 covering wide ranges from < 1 µg g-1 to 100%; and (4) it is a common laboratory
915 instrument and therefore readily accessible. Therefore, XRF plays an important role in
917 preparation process and quick measurements of multi-element within a few minutes
918 [217,218]. Depending upon the detector types, there are general two XRF techniques,
921 analysis, WDXRF shows better performance in analysis of trace REY in solid
922 materials, including coal ash [219–221]. However, several problems occur in REY
52
925 Spectral interferences
928 Therefore, the use of XRF techniques for quantifying REY in coal ash is not as
929 popular as other three instrumental methods (Figure 8). For REY analysis in coal ash,
930 the most serious problems of WDXRF are probably matrix effects and overlapping of
931 the analytical lines. For example, the signals of HREE in coal ash may be weakened
932 (absorption effects) because of the absorption of X-rays by light rare earth elements or
933 other major elements in coal ash. In a study by Eze et al. [186], only Sc, La, and Ce
934 were detected by XRF due to no suitable standards for calibration. Table 8 listed the
935 possible interfering lines in the XRF analysis of REY in coal ash. Smoliński et al.[219]
936 developed a method for the quantification analysis of REE based on WDXRF. The
937 matrix effects and spectra interferences during REY determination are corrected by
938 calibration and peak de-convolution of the overlapping spectral lines. Based on the
939 analysis of 16 REY in 12 different coal combustion ash and eight certified reference
940 materials, the relative standard deviations (RSD) and the recoveries of most REY in
941 the standard ash samples are estimated to be 2.1-12.9% and < 10%, respectively.
942 However, the recovery rates of Tb (21.8%), Dy (21.8%), and Er (20.1%) in the
943 standard ash are not satisfied. This is mainly caused by the lower concentrations of
944 HREE in coal ash and thus the Lα lines (2θ angles of Tb and Dy: 56-58°) are easily
945 interfered with Fe Kα (2θ angles: 57.5°) and Fe Kβ lines (2θ angles: 51.7° vs 52.6° of
53
946 Lα line of Er). In general, the study from Smoliński et al. [219] demonstrated that the
947 WDXRF can be used to estimate most REY in coal combustion ash.
948 Portable XRF is generally used as a screening tool in field geological and
950 ores, rocks, sediments, etc., [222–227]. To quickly identify REY-rich coal or coal ash
951 in the U.S. coalfield and power plants, Bryan et al. [218] studied the use of a portable
952 hand-held XRF to estimate the concentrations of REY. Generally, the results of LREE
953 content obtained from the portable XRF units could be correlated to the laboratory
954 quantitative analysis, with a correlation coefficient of 0.878. Thus, it can be used to
955 screen likely samples for submission to the laboratory. The accuracy, however, is not
956 quantitatively reliable. For example, the detected Y contents in the NIST 1633c via
957 the portable XRF were 5-7 times higher than the certified values.
958
959 Table 8. Lines for REY determination, potential spectral interferences, and analysis
960 uncertainty of REY by XRF technique. Revised after Smoliński et al. [219].
Sc Kα 97.74 96.10 /
La Lα 82.88 84.36 /
54
Sm Lα 66.2 67.08 Lβ2Ce
961
962 Overall, a general conclusion can be reached is that the main analytical
963 techniques have been used for REY determination in last twenty years are ICP-MS,
964 ICP-OES, INAA, and XRF (Figure 8). A comparison of these analytical methods in
965 REY determination in coal ash is summarized in Table 9. Coal ash usually contained
966 low concentration of individual REY (sub-μg g-1 to μg g-1 range) and the major
967 chemical components and inorganic salts could bring matrix effects, spectral
968 interferences, and other instrumental problems for the four analytical techniques.
969 ICP-MS is recommended for determining REY in coal ash because of its high
970 sensitivity, multi-elemental capability, and reasonable costs. The measurement of REY,
971 especially low content HREE by ICP-MS is critical because ICP-MS can directly
972 determine the digestion solutions without separation and pre-concentration procedure.
55
973 As mentioned in 3.1.3, in terms of HREE determination, several methods can
974 overcome the spectral interferences during the ICP-MS analysis of HREY in coal ash
975 digestion solutions: i) monitoring the isobaric REE interferences from oxides of
976 lighter REE (La, Ce, Pr and Nd)) or other elements (BaO and BaOH) on the HREE,
977 for example using the mass ratio of CeO/Ce or ThO/Th, and the value should be kept
978 < 2%, ii) the use of collision cell by introducing pure gas (such as helium) to
979 eliminate the polyatomic and doubly-charged interferences, iii) algebraic correction
980 that can be used to reduce overlapped spectra lines, for example the interference of
981 PrO and NdO on Gd and Tb. In contrast, pre-concentration and matrix separation
982 might be necessary prior to ICP-OES analysis (especially for HREE), for the coal ash
983 containing REY at normal concentration level (contents of total REY below 300 μg
984 g-1). Further work should develop workable pretreatment methods to overcome these
985 problems. INAA could be a reference method for assessing the precision and accuracy
987 method for analysis of solid sample, is suitable used for exploring REE-rich coal ash
56
989
990 Table 9. A comparison of the four main instruments (ICP-MS, ICP-OES, INAA, and XRF) for REY determination in the published literature
991 [150,151,186,202,204,209,218,228].
57
992 3.2. Speciation analysis
994 Speciation of REY in coal ash assists in understanding their partitioning behavior
995 in coal combustion process and inform REY recoveries strategies [26,229–232].
996 Methods that are used to measure REY occurrences in coal ash can be classified into
997 indirect methods and direct methods (Figure 7). Indirect methods refer to applying
998 the method of statistical calculations, physical separations, and chemical leaching to
1000 Statistical calculation can provide preliminary but limited REY speciation
1002 magnetic separations are methods for REY separation from bulk fly ash
1004 beneficiation and pre-concentration of REY from fly ash for the further extraction,
1005 having few implications for REY occurrences. The detailed descriptions can be
1006 referred to section 7. Here, we will focus on making a review on the chemical
1007 leaching methods, since it is an effective process to quantify REY speciation and have
1009 Sequential chemical extraction (SCE) has been extensively used for determining
1010 trace elements associations in coal fly ashes. As shown in Table 10, numerous
1011 sequential leaching protocols were designed to study the REY speciation in coal ash
58
1014 Easily-leached fraction: including the water-soluble, ion-exchangeable, and weak
1015 acid-soluble forms, which can be easily released with mild regents such as
1016 deionized water, ammonium acetate, magnesium chloride, dilute HCl, acetic acid,
1021 requires relatively strong acid or chelating agents (e.g., oxalic acid); and
1024 The major problems of SCE process may arise from the assumption that each
1025 chemical reagent reacts with a special REY-bearing phase. However, this might be
1026 not true in many cases because REY can be leached from multiple phases [145]; and
1027 secondary reactions (e.g. re-adsorption, precipitation, and re-dissolution) may occur in
1028 the leaching steps. Therefore, it is suggested that each step of the SCE process should
1029 be theoretically and/or experimentally verified. As shown in Table 10, Liu et al. [145]
1030 proposed a three-step sequential acid leaching procedure for discerning REY
1031 associations in coal ash. The procedure was validated by the acid leaching
1032 experiments with REY reference compounds and the thermodynamic prediction of
1034 PHREEQC. This procedure may be suitable to quantify REY occurrences in fly ashes.
1035 Note that the predicted dissolution curve of some REE-bearing phases by PHREEQC,
59
1036 for example the complete dissolution of monazite at pH = 1.0 seems to be unrealistic
1037 [229]. As indicated by Liu et al. [145], the ash compositions, particle size, and
1038 physical distribution of REY-bearing minerals can affect the REY dissolution kinetics.
1039 Overall, a reliable and convincing quantification of REY species in fly ash by
60
1041 Table 10. A summary of various sequential chemical extraction methods used for determining REY speciation in coal fly ash samples.
4-step sequential ion-exchangeable, acid soluble, metal oxides, organic or sulfide, 75-77% REY bound to silicate and aluminosilicate, with minor [108,121]
extraction and silicate/aluminosilicate form fraction being acid soluble and organic/sulfide form
7-step sequential water soluble, exchangeable, carbonate-bound, Mn 86.1% of REE were associated with the residual phase [176]
HCl leaching leached by cold dilute HCl (HCl: H2O =2:1), HCl soluble and about 50–55% solubility of Y for the fluidized coal ash, higher than [20]
4-step sequential leaching water leachable, ion-exchangeable form, acid soluble form, low mobility (< 30% extractable fraction) in fly ash relative to the feed [171]
metal oxides form, organically or sulfide form, and residual coal, REY maybe incorporated in high-temperature aluminosilicate
phases
sequential leaching REE oxides and REE carbonates dissolved at pH 5.5−4; apatite Class F fly ash: 30-70% of REE are associated with the zircon and [145]
61
dissolved at pH 3.5−2; REE phosphates and hematite dissolved glass phase, 10-40% in apatite, 10% with oxides and carbonates, 10%
at pH < 1.5, and zircon and glass phase with phosphates and hematite; Class C fly ash: 50−60% of REEs are
and hematite
HF leaching 4% HF solution was used to tentatively separate the glassy phase <10% of REY retained in the undissolved crystalline phases, with [27]
and crystalline phase more LREY than HREY; and over 90% of REY are associated with the
magnetic using magnetic separation - 30% NaOH - 15% HCl to separate REE are enriched in glassy phases and depleted in crystalline minerals [119,234]
revised BCR method water soluble (F1), exchangeable/acid soluble (F2), reducible The sum of the F1, F2, F3, and F4 in PRB ash (> 60%) is much higher [233]
(F3), and oxidizable (F4) than in App ash and IL ash (< 15%)
62
4-step sequential ion exchangeable, carbonates, metal oxides, acid soluble, and the majority of REEs in the calcined samples (600-750℃) occurred as [159,163]
extraction insoluble/silicates metal oxides, HREEs were more likely associated with easily
1042
63
1043 3.2.2. Direct microanalysis methods
1044 In recent years, to develop effective REY recovery techniques, there are a
1045 number of studies working on in-situ identifying and quantifying REY speciation in
1047 As summarized in Figure 7, these direct methods are generally divided into:
1049 secondary ion mass spectrometry (SIMS; also called ion microprobe analysis);
1052 (EPMA), focused ion beam and scanning electron microscopy (FIB-SEM),
1054 selected area electron diffraction (SAED), fast Fourier transform (FFT), and
1060 SEM-EDS can be used to determine REY occurrences in fly ash powder or
1061 polished pellet. REY-bearing phases usually appear to be very bright in the ash pellets
1062 at backscattered mode, since the brightness of the backscattered imaging depended on
1063 the average atomic number of the material. As a result, SEM-EDS is capable of finding
1064 discrete REY minerals that are dispersed in coal ash [122,144,147,192,236]. EPMA is
64
1065 similar in scope to the SEM methods, and one of the main differences between the two
1066 methods is that element concentrations can be accurately quantified by the wavelength
1067 dispersive spectrometry (WDS). EPMA has significantly lower detection limits
1068 (~0.01wt.%) for REY relative to EDS (~0.1wt.%) and is thus more capable of
1069 determining the dispersed occurrences of REY in trace phases [146,147,192]. However,
1070 the bulk analysis indicated that the concentration of individual REY in coal ash is
1071 generally lower less than 100 μg g-1, especially for some low-content HREE being far
1072 beyond the detectability of EPMA. In addition, REY mineral phases are very
1073 complicated, one single particles (several microns in diameter) may contain nanoscale
1074 multiple REE-bearing phases [144,233]. Detailed and accurate information on trace
1075 REY phase in coal ash can be obtained with TEM and other micro-scale mass
1077 TEM and related techniques to determine REY occurrences in fly ash have been
1079 examination of coal ash by SEM-EDS and EPMA lay foundation for the use of these
1080 advanced techniques. After the SEM-EDS survey of a small quantity of coal ash,
1081 REE-rich particles are identified and localized, then the individual minerals or mineral
1082 assemblages of interest can be isolated and extracted through in situ Focused Ion
1083 Beam (FIB) technology. Following FIB extraction, the lift-out samples are mounted
1084 on a Cu grid and ion milled to 100 nm or less for the TEM analysis. Selected area
1085 electron diffraction (SAED) is employed for mineralogy identification of the selected
1086 grains; and fast Fourier transform (FFT), computed by image analysis software, is
65
1087 used to determine the lattice spacing in HRTEM micrographs. Chemical identification
1088 in TEM is available in some units via electron energy loss spectroscopy (EELS) and
1090
1091 Figure 9. A general diagram showing how the transmission electron microscopy
1092 (TEM) and related techniques work on identification of REE-bearing grains in coal
1093 and coal fly ash. After Hower et al. [231,236]. Reproduced with permission from
1094 Elsevier.
1095
1096 The microanalysis based on mass spectrometric techniques have been widely used
1097 in trace element geochemistry study of inorganic minerals and rocks [239–243]. A
1098 major difference in these microanalysis techniques is the rate and depth of penetration
1099 within the sample. In LA-ICP-MS, solid samples are ablated with a laser source to tens
1101 compositional variation with sample depth. Application of LA-ICP-MS to coal ash
1102 aims principally at quantifying the spatial distribution and association of elements in
66
1103 coal fly ash. Spears [244] Bauer et al. [245], and Kostova et al. [246] used
1104 LA-ICP-MS [244] to determine the major element contents in epoxy-mounted coal fly
1105 ash samples. Piispanen et al.[246] compared the LA-ICP-MS results of major
1106 elements in fly ash samples to the results by SEM-EDS, finding a consistent result
1107 between the two methods. Trace elements of environmental concern, such as As, Se,
1108 and Pb, have been successfully determined in fly ash pellets by LA-ICP-MS, as
1109 reported by Spears [244]. For REY determination, Hood et al. [192] applied
1110 LA-ICP-MS to determine the concentration of Sc, Y, La, Ce, Pr, Nd, and Sm in a set
1111 of fly ash samples derived from Kentucky Fire Clay coal using NIST SRMs 610, 612,
1112 and 614 as calibration standards. The matrix and the homogeneity of NIST reference
1113 materials differ from that of fly ash so that the results are semi-quantitative.
1114 Thompson et al. [237,247] explored the use of varying laser spot size (32-60 μm) to
1115 determine the REY concentration in coal fly ash. Instead of selecting a specific
1116 element as an internal standard, the quantification of REY in randomly selected laser
1117 spots were achieved by normalizing all elements to 100% against NIST SRM 610
1118 glass reference. The overall average REY concentration of the randomly ablated spots
1120 Recent studies have tried to use SIMS to discern REY and other rare metal
1121 occurrences in coal ash. For example, like REY, lithium (Li) is also a critical metal
1122 which might be recovered from some coal ash. To gain insights on the speciation of Li
1123 in coal ash, Hu et al. [248] used SIMS to analyze the distribution of Li in high-Al coal
1124 fly ash, using Bi1+ or Bi3++ as the primary ion beam with a spot size of 0.2 μm. In SIMS,
67
1125 a primary beam of incident ions sputters secondary ions from the sample at a much
1126 slower rate, typically leading to penetration depths of only about 1-5 µm. Compared to
1127 smaller ion microprobes, the SHRIMP-RG (Sensitive High Resolution Ion Microprobe
1128 – Reverse Geometry) ion microprobe and other SHRIMP configurations employ a large
1129 format magnetic sector mass spectrometer with high mass resolution, thereby
1130 minimizing the effect of isobaric interferences in SIMS analysis. Kolker et al. [146]
1131 analyzed REE distribution and occurrences within ash particles using Stanford-USGS
1132 SHRIMP-RG ion microprobe. An oxygen negative-ion beam with spot size of 15 μm
1133 was used to quantify eleven REE in 19 US and international coal fly ashes. NIST
1134 glass standards (SRM 611 and 613) were used as internal standard for calibration and
1135 the overall analytical uncertainty for REE was reported to be within 10–20%.
1137 species and interparticle distribution differences in complex ash matrices. SEM-EDX
1138 and EPMA are the most common techniques used for geochemistry study in many
1139 laboratories but have limited detection limits and lower resolution (compared to TEM)
1140 for analyzing trace metals in coal ash. For REY determination, these two methods can
1141 be used as preliminary steps for other advanced microscale techniques, such as TEM,
1142 LA-ICP-MS, and SIMS. In both LA-ICP-MS and SIMS, they have appropriate
1143 detection limits at the µg g-1 to sub-µg g-1 level, which is important to characterize
1144 grain-scale REY distribution in coal ash. However, a major problem of these two
1145 methods is obtaining a calibration standard which should be: (1) homogenous on a
1146 grain scale, (2) a good matrix match to the material being analyzed, and (3) avoid
68
1147 spectral interferences of other isotopes [239,244,249]. In addition, the working spot
1148 size of LA-ICP-MS or SIMS might be too large to distinguish REY associations in the
1149 fly ash particles. These large-scale techniques gloss over the actual mineral and
1150 (potentially) non-mineral associations at nanoscale. TEM and related techniques, such
1151 as SAED can provide more details of REY occurrences in the nanoscale examination,
1152 which is an important supplement to the association of REY in coal fly ash.
1155 discern the speciation of REY in coal ash. For those elements of relatively high
1156 abundance in fly ash samples (such as La, Ce, Nd, and Y), X-ray absorption
1157 spectroscopy of a fly ash sample can be used to assess bulk-level element speciation.
1158 For example, bulk XANES has been used to identify major phases of Ce and Y,
1159 primarily through linear combination fitting (LCF) models of the sample spectrum with
1161 percentages of the element as different reference species. This approach generally
1162 requires careful selection of known reference materials that could be reasonable
1163 approximations of the elemental forms in fly ash. Thus, the selection of reference
1164 materials must consider the conditions of fly ash formation and collection. The
1165 selection process can be especially challenging if the individual elements are
1166 distributed diffusely within aluminosilicate glasses. In this case, the localized
1168 material (see section 6.4), and is not easy to mimic in laboratory-synthesized materials.
69
1169 The utility of XANES analyses is often limited by the relatively high
1170 concentration requirements of the method, particularly as coal fly ash is also enriched
1171 in other elements that might be interfering (Table 11). Quantitative identification of
1172 REY species also requires sufficient differences in the spectral features of candidate
1174 yttrium K-edge XANES for coal fly ash, the spectral features of an yttrium carbonate
1175 mineral (Y2(CO3)3·3H2O) and monazite standard were remarkably similar to Y-doped
1176 glass and monazite reference materials (Figure 10). Thus, in the fitting of XANES
1177 spectra for coal fly ash samples, the replacement of one of these references with the
1178 other did not substantially alter the quality of the model fits. These subtleties emphasize
1179 the need for careful and cautious interpretation of XANES results. In other words, often
1180 the results are limited to qualitative descriptions rather than quantitative interpretations.
1181 In addition to XANES technique, the use of EXAFS spectroscopy can determine the
1182 local bonding environment of the absorber atom (~5 Å) and provide structural
1183 information such as coordination number and bond distance that can differentiate
1184 compounds (e.g., between Y-O and Y-P structures) and complement results of XANES
1185 analysis. However, due to the low REE concentrations and line inferences, there have
1186 been no study for REE in coal fly ash using EXAFS. Therefore, more work with
1187 EXAFS or other similar bulk elemental speciation methods is required to improve the
1189
70
1190 Table 11. Rare earth elements in coal fly ash that could be analyzed for bulk
1192 consider in coal fly ash. Data from Taggart et al. [233].
Potential
Concentration in fly Absorption Emission
Element interfering
ash energy energy
elements
5732 eV 4840.2 eV
-1
Cerium (Ce) 100 – 200 µg g V, Ba
(L3-edge) (Lα1)
5483 eV 4651.0 eV
-1
Lanthanum (La) 70 – 110 µg g Ti
(L3-edge) (Lα1)
6208 eV 5230.4 eV
-1
Neodymium (Nd) 60 – 90 µg g Possibly Ce
(L3-edge) (Lα1)
17038 eV 14958 eV
-1
Yttrium (Y) 80 – 100 µg g None likely
(K-edge) (Lα1)
71
1193
1194 Figure 10. Bulk Y XANES spectra for yttrium reference compounds. Note t
1195 hat the spectral features for the Y-doped glass, monazite, and Y2(CO3)3∙3H2O wer
1196 e similar to each other. After Taggart et al. [233]. Reproduced with permission fr
1197 om the Royal Society of Chemistry. Further permissions related to the material ex
1199 g/en/content/articlelanding/2018/EM/C8EM00264A.
1200 A summary and comparison on the advantages and limitations of various methods
1201 for determining REY speciation is given in Table 12. As shown in Table 12, the
1202 identification and quantification of REE in coal ash is still challenging due to low REY
1203 contents and complex ash matrices. One should keep in mind that due to the limitations
72
1204 of each method; no single scale/ technique can provide all of the answers. Depending
1205 on the ash properties (particle size, crystallinity, REE contents, and among others),
1206 readers should be cautious to the speciation results derived from different analytical
1207 techniques. Comprehensive results from both indirect and direct methods are
73
1209 Table 12. A comparison of direct and indirect methods on REY speciation analysis.
SEM-EDS Submicron Chemical analysis of areas of interest; Particle ~ 0.1wt.% Low spatial re
EPMA Submicron Chemical analysis of areas of interest; lower ~ 0.01wt.% Low spatia
SIMS Submicron Low detection limit at μg g-1 or sub-μg g-1 level; sub-μg g-1 Working sp
LA-ICP-MS Submicron Low detection limit at μg g-1 or sub-μg g-1 level; sub-μg g-1 Working sp
74
distribution of REY within ash at trace level
Bulk XANES Bulk Oxidation states of REY; Quantification of ~ 0.01wt.% High detectio
fitting problem
Sequential Bulk Quantification of REE associations; low cost Depending on the analytical instruments Quantifica
Physical Bulk Preliminary information of REE affinity Depending on the analytical instruments
separation
1210
75
1211 4. Concentrations and valuation of REY in coal ash
1213 In the review by Ketris and Yudovich [82], the average REY content in the world
1214 coal ashes is estimated to be 404.5 µg g-1, approximately three-times greater than that
1215 in the earth’s crust (180.9 µg g-1). However, the results from Ketris and Yudovich [82]
1216 were the equivalent value of REY in coal on an ash basis, rather than the determined
1217 values in real coal combustion ash produced at power plants. In order to better
1218 evaluate the reserve of REY from the existing coal combustion ash, current study
1219 compiled data of 581 ash samples derived from different coal-fired power plants in 15
1220 countries (Table 13). Considering the number of samples available from each country,
1221 six countries including Spain, England, Poland, Bulgaria, Romania, and Finland are in
1222 the group of Europe; and four countries including South Africa, India, South Korea,
1223 and Indonesia are classified into the group of “other countries”. As a result, the
1224 average concentration of REY in world coal ash is estimated to be 435.45 µg g-1,
1225 slightly higher than the reported value by Ketris and Yudovich [82]. Coal ash of China
1226 (473 µg g-1) and the U.S. (459.61 µg g-1) contains higher contents of REY than that of
1227 Europe (278.65 µg g-1) and other countries (298 µg g-1). This might be caused by the
1228 limited number of samples from these two regions, where no data is available on the
1229 coal ash generated from the combustion of coals containing high REY contents. The
1230 rare earth oxides (REO) have been used as a proxy for estimating the abundance of
1231 metals in ores. Some coal ash, for example, fly ash from Eastern Kentucky
1232 pulverized-coal fired power plants [250] has been reported to have extremely high
76
1233 REE concentrations (1202-1667 µg g-1), comparable to the REO content of some
1234 conventional REE ores, such as the ion-adsorbing type rare earth ores and low-grade
77
1236 Table 13. A summary of the abundances of REY in coal ash from different countries around the world. Unit: µg g-1
a b c d e
China US Europe Others World
average range n average range n average range n average range n average range n
Y 57.4 1.5-233.0 217 68.2 6.2-214.0 257 33.1 5.1-60.7 72 36.4 2.2-77.0 20 58.5 1.5-233.0 566
La 84.4 5.8-441.0 224 73.5 21.9-265.0 257 45.0 2.6-103.0 80 54.5 9.6-112.0 20 73.1 2.6-441.0 581
Ce 176.8 21.9-955.0 224 161.6 44.0-534.0 257 98.7 5.2-221.0 80 103.6 16.2-222.0 20 156.8 5.2-955.0 581
Pr 19.1 2.7-117.0 224 17.2 0.10-63.0 257 11.2 0.7-26.0 80 14.5 2.3-48.0 20 17.0 0.1-117.0 581
Nd 75.3 9.7-436.0 224 74.3 21.4-234.0 257 56.2 3.1-264.0 80 44.3 8.8-86.5 20 71.2 3.1-436.0 581
Sm 13.7 1.7-79.0 224 14.3 4.4-50.5 257 8.6 0.5-16.0 80 11.1 1.7-53.0 20 13.2 0.5-79.0 581
Eu 2.5 0.3-8.0 224 3.0 bdl-7.0 257 1.9 0.2-4.0 80 2.1 0.5-3.5 20 2.6 bdl-8.0 581
Gd 14.1 1.7-73.0 224 14.8 4.6-40.4 257 9.3 0.5-20 80 8.0 1.8-16.8 20 13.5 0.5-73.0 581
Tb 2.0 0.17-11.0 224 2.3 0.7-6.6 257 1.6 0.1-7.0 80 1.4 0.3-2.51 20 2.0 0.1-11.0 581
Dy 11.3 0.9-55.0 224 12.3 3.8-44.2 257 7.0 0.5-15.0 80 7.4 1.5-14.2 20 11.0 0.5-55.0 581
Ho 2.2 0.2-11.0 224 2.2 0.1-8.8 257 1.2 bdl-2.9 80 1.7 0.3-2.9 20 2.1 bdl-8.8 581
Er 6.5 0.4-31.0 224 7.7 2.2-24.5 257 4.4 0.3-15.0 80 11.0 0.9-120.0 20 6.9 0.3-120.0 581
Tm 0.9 bdl-5.0 224 1.0 bdl-6.0 257 0.5 bdl-1.1 80 0.8 0.1-1.6 20 0.9 bdl-6.0 581
Yb 5.9 0.3-30.0 224 6.5 2.1-21.8 257 3.9 0.4-9.0 80 4.3 0.8-7.8 20 5.8 0.3-30.0 581
Lu 0.9 bdl-5.0 224 0.9 bdl-3.0 257 0.6 bdl-2.0 80 0.9 0.1-2.0 20 0.8 bdl-5.0 581
LREY 371.5 62.9-2028.0 340.8 101.6-1140.7 218.8 12.1-630.0 226.7 42.6-463.1 331.3
MREY 86.5 7.4-380.0 100.5 30.94-299.4 49.4 1.3-91.0 54.3 13.3-114.0 29.2
HREY 16.5 1.4-82.0 18.3 5.7-61.0 10.4 0.9-25 17.1 2.4-122.0 16.5
TREY 473.0 74.1-2490 459.6 117.3-1295.3 278.7 14.3-4884.0 298.0 58.2-597.9 435.5
Critical
0.39 0.30-0.76 0.37 0.28-0.5 0.34 0.24-0.48 0.35 0.24-0.51 0.36 0.24-0.76
REY ratio
a
1238 China [24-28, 107, 108, 119, 121, 160, 161, 169, 178-180, 196, 234, 252]
b
1239 US [12, 15-17, 42, 120, 122, 140, 144, 145, 146, 147, 158, 167, 191, 231-233, 238, 250-251, 258-259, 262, 264, 271 ]
c
1240 Europe [18-23, 97, 166, 168, 170, 171, 186, 191, 213, 246]
d
1241 Others [31-33, 185]
e
1242 World [82]
1243
78
1244 4.2. REY contents in coal ash from major coal-producing countries
1246 The concentration of REY in coal ash is largely dependent on the geological
1247 origin of the parent coal. The burning of coal from some coal-hosted ore deposits can
1248 further enrich REY in coal ash and may produce the potential “artificial REY ores”
1249 (REY-rich coal ash). Thus, prioritization of ash sources for REY recovery requires a
1250 detailed knowledge on REY concentrations of different types of coal ash from
1251 different origins or regions. The information is also vital in order to explore possible
1252 strategies to leach REY from the ash during recovery operations and understand the
1253 potential valuation of the coal ash with respect to the REY reserves. In view of this,
1254 previous findings in the published literature are summarized and discussed in the
1255 review, with emphasis on ash samples from U.S. and Chinese power plants as two
1256 examples.
1257 Extensive analysis of REY contents has been performed on ash samples from
1258 U.S. power plants (Table 13). Taggart et al. [16] made a broad survey study of REY
1259 contents in over 100 U.S. coal fly ash samples produced from coals from three major
1260 coal basins, namely the Appalachian basin, Illinois basin, and Powder River basin
1261 (Figure 11A). The total REY content and trends in the U.S. fly ashes are:
1262 REY contents differed significantly by coal basins, showing a decreasing order of
1263 Appalachian basin coal ash (591 µg g−1) > Illinois Basin coal ash (403 µg g−1) >
79
1265 Relative to the UCC, REY distribution pattern of coal fly ash displayed different
1266 enrichment modes among the three basins, suggesting the characterization of
1267 REY in coal ash mainly inherited from the feed coals.
1268 Afterwards, fly ash samples from burning Illinois basin and Powder River basin have
1269 been detailed investigated by Hower et al. [251] and Huang et al. [120], respectively.
1270 The results confirmed the REY contents for Illinois Basin coal-sourced and Powder
1271 River basin coal-sourced fly ashes were less than those of Central Appalachian
1272 coal-sourced fly ashes. Meanwhile, a scattered distribution of the REY in coals of
1273 each region is also observed due to the mine-to-mine variations of REY contents in
1275
1276 Figure 11. Comparison of total REY contents (A) and the critical REY ratios (B) in
1277 coal combustion ash at power plants from three major U.S. coal basins: Appalachian
1278 basin (App, triangles in blue), Illinois basin (IL, circles in red), and Powder River
1279 basin (PRB, diamonds in black). After Taggart et al. [16]. Reproduced with
1280 permission from the American Chemical Society. Further permissions related to the
80
1281 material excerpted should be directed to the American Chemical Society at
1282 https://pubs.acs.org/doi/abs/10.1021/acs.est.6b00085.
1283
1284 For Chinese coal ashes, compiled data from published literature on REY
1285 concentrations from different provinces and/or regions from China is discussed. A
1286 total of 227 sets of data related to REY analysis (including 11 samples from the first
1289 contents in coal ashes among different provinces or cities of China is compared
1291 Based on the available data and the geographic locations, provinces with
1292 different REY concentrations in coal ashes can be divided into three zones (Figure
1293 12). The total REY differed among these zones, following the decreasing order of
1294 Zone Ⅰ (623.5 μg g-1) > Zone Ⅱ (430.9 μg g-1) > Zone Ⅲ (318.6 μg g-1). Zone Ⅰ
1296 Chongqing, Yunnan, and Guizhou). This is consistent with the distribution of REY
1297 contents in Chinese coal basins, where feed coals mined from the southwestern China
1298 are rich in REY. Zone Ⅱ consists of five provinces from central China (Shanxi,
1299 Shandong, Henan, Hubei, and Anhui); and one province from southern China
1300 (Guangdong province) is also included, because the feed coal for power generation is
1301 mainly derived from the central regions (e.g., Shanxi province). REY concentrations
1302 in coal ashes from Zone Ⅱ are much lower than that of Zone Ⅰ. Inner Mongolia and
81
1303 Xinjiang autonomous regions, as two important coal producing area located in the
1304 Northeastern and Northwestern China are grouped into Zone Ⅲ. Although some coals
1305 from Inner Mongolia, such as REY-rich Pennsylvanian coals from Jungar and
1306 Daqingshan coalfields are reported to have high concentration of REY [254], the
1307 compiled results at present study suggest that REY are not significantly enriched in
1308 the coal ashes from Zone Ⅲ. This is probably caused by (i) the “mineralized coal”
1309 from Zone Ⅲ fed into the utility boilers depleted REY and (ii) insufficient published
1310 data related to the abundances of REY in the coal ashes from this region.
1311
1312
1313 Figure 12. Distribution of rare earth elements in coal ash across China. Data was
1315
1317 In addition to the total REY concentration, the ratio of critical rare earth element
1318 (selected MREY and HREY) is another important parameter influencing the potential
82
1319 values of rare earth ores. As shown in Table 13, the average ratio of critical REY (Nd,
1320 Eu, Tb, Dy, Y, and Er) in the world coal ash is 36%, which is higher than some
1321 conventional REY ores. Accordingly, coal ashes that are enriched in critical REY
1322 would provide alternative sources to the conventional rare earth ores.
1323 Similar to the REY contents, the critical REY fraction also heavily depends on
1324 the origins of feed coal. For the U.S. coal ashes, the critical REY fraction was greatest
1325 for the Appalachian basin and Illinois basin-sourced coal ashes (Figure 11B) than
1326 ashes from Powder River basin. There are no statistically differences in the critical
1327 REY ratios between Appalachian basin and Illinois basin coal ashes [16].
1328 The ratio of critical REY in different zones in China is displayed in Figure 13.
1329 The data demonstrated that the critical REY content differed significantly among the
1330 three regions (Kruskal-Wallis test, p = 0.005). Ashes from Zone Ⅱ had higher critical
1331 REY ratios than those from Zone Ⅰ (median difference of 3.4%) and Zone Ⅲ (median
1333 REY of Chinese coal ashes is higher than that of selected conventional REE ores
1334 currently being mined, such as the super large Bayan Obo Fe-REE-Nb ore deposit in
1335 Inner Mongolia of China (< 10% critical REY). As shown in the UCC normalization
1336 curve of REY in coal ash, REY in coal combustion ash show a medium- and heavy-
1337 REY distribution pattern, which is different from the typical REE ores (LREE rich
1338 type).
1339 Overall, both of the total REY and critical REY contents are mainly determined
1340 by the origin of feed coals. Coal ash samples produced in U.S. and China would
83
1341 provide three times the critical REY of total REY extracted per kg than that of
1342 conventional ores. The high fraction of in coal ash may represent a major advantage
1343 over the conventional ores if the extraction costs per kg of can match that of REE
1345
1346
1347 Figure 13. The ratio of critical-to-excessive REY in China coal ashes from different
1348 zones (A) and the normalization curve relative to UCC (B). Data was compiled from
1350
1353 The “workable reserve” of REY in coal combustion ash depends not only on
1354 their concentration but also on the quantity of available ash. In the United States,
1355 around 59.6% of the 45.7 Mt of coal combustion ash produced annually in the US is
1356 beneficially reused, whereas the remainder was generally discarded [255]. Taggart et
1357 al. [16] estimated that the annual production of REO in unused portion of coal fly ash
1358 was 4000 t for the Appalachian Basin, 1280 t for the Illinois basin, and 3630 t for the
84
1359 Powder River basin. The unused fly ash comprises a REY reserve that is similar in
1360 scale to the annual production of REY at the Mountain Pass mine (4769 tons in 2014).
1361 China is the world’s largest consumer of coal, with annual usage surpassing that
1362 of the US, Japan, and European Union combine [256]. Annual amount of generated
1363 combustion residual from thermal power plant is huge. In 2017, about 70% of 686 Mt
1364 was reused for beneficial purposes [257]. The remainder is disposed in landfills and
1365 thus the annual ash production plus the fly ash already in storage constitute a huge
1366 potential REY resource. Based on Taggart et al. [16], this study made an similar
1367 assessment of REY reserves in the unused coal ash annually produced by Chinese
1368 power plants. Assuming that coal-fired power generation of each provinces mirrors
1369 the relative coal ash production by region, then the annual total amount of coal ash
1370 produced from the Zone Ⅰ, Zone Ⅱ, and Zone Ⅲ was estimated to be around 32.8,
1371 260.5, 90.0 million tons; and the amount of unused ash accounted for 30% of the total
1372 ash, that is, 9.8 million tons for Zone Ⅰ, 78.2 million tons for Zone Ⅱ, and 27.0 million
1374
1375 Table 14. A summary of annual coal ash production, unused ash amount, annual
85
Power
kW•h
Inner 90,028,186
3750 8.0 55,176,259
Mongolia
1377
1379 Based on the data in Table 14, the annual total tonnage of REO in the discarded
1380 coal ash is estimated to be 8029 t for the southwestern provinces of Zone Ⅰ, 42,114 t
86
1381 for the central provinces of Zone Ⅱ, and 9769 t for Zone Ⅲ, respectively. If all of
1382 REO in the unused coal ash is extracted, the total amount could be around 59,909 t
1383 (Table 14). This coal ash reserve of REO annually (the year of 2019) produced from
1384 China power plants is nearly half of the annual China REY mine production (132
1386 https://www.statista.com/statistics/268011/top-countries-in-rare-earth-mine-productio
1387 n/). According to the 2020 prices for REO (http://www.reht.com/h-nd-426.html), the
1388 total value of the REO in the discarded ash reserve from China is estimated at 14.8
1389 billion yuan (Table 15), which is equivalent to U.S. 2.2 billion dollars based on the
1390 annual average exchange rate of Chinese Yuan to US dollar (0.15 USD). The REY
1391 value in Chinese coal ash is lower than that of US coal ash as estimated by Taggart et
1392 al. (4.3 billion dollars) [16]. Main reasons are the large variations of REY prices with
1393 time, different REY contents (especially critical REY) and Sc is excluded from the
1394 valuation due to insufficient Sc data in coal ash. Note that only a part of coal ash
1395 could be extracted for rare earths products, as indicated by the large variations of REY
1396 concentration in different coal ashes [258]. Accordingly, the valuation of REY
1397 reserved in coal ashes is likely smaller since not all of the unused ash can meet the
1398 requirements of being used as extraction sources. Besides the total value, the value of
1399 REO per ton of coal ash was also calculated to provide a basis for assessing the use of
1400 coal ash as an alternative REY source. As shown in Table 15, it is estimated that the
1401 per-ton REO values is 180.1 yuan for Zone Ⅰ, 111.9 yuan for Zone Ⅱ, and 66.3 yuan
1402 for Zone Ⅲ. The main contributors to the value of REO are some of the critical rare
87
1403 earths. The high prices of Nd (374 yuan/kg), Tb (4950 yuan/kg), and Dy (1950
1404 yuan/kg) contribute to near 70% of the total value of the whole REY value in coal ash.
1405 The result highlights the importance of the high ratio of critical REY in ash, which is
1406 one of the main advantages over other conventional rare earth ores.
1407 Overall, the value of REY in coal ash primarily depends on several factors, i.e.,
1408 the total REY concentration in coal ash, the ratio of critical REY, the separation
1409 technology, and the global market price of REO [18,281,295]. The valuations will be
1410 adjusted, depending upon these factors especially the extraction techniques that are
1411 currently developed. The costs for REY recovery from coal ash, such as transportation
1412 and extraction processes, should be scaled regarding the valuation. To add values and
1413 reduce the overall costs, the selection and pre-concentration of REY-rich coal ash as
1414 well as co-extraction of other metals or reuse the wastes after extraction should be
1415 considered and incorporated in the extraction procedure (see the discussion in section
1416 7). There are huge amounts of “old ash” preserved in landfill sites (e.g., ash ponds),
1417 that have been accumulating for many years could be a source but is not considered in
1418 the valuation. Considering the state of the coal-fired generating industry (continues to
1419 fall) in the developed countries, such as in the U.S., this preserved ash would be a
1420 more viable resource. Waste management regulations would additionally drive the
1421 scientific community and relevant enterprises to explore the REY recovery from coal
1422 ash, particularly for the REY-rich ash disposed in potential agriculture lands [16,122].
88
1423 Table. 15. Total mass and estimated value of REO as well as the REO value per metric ton of fly ash produced annually in China.
a
Total REO (t/yr) Total mass 2020 prices Total value Chinese yuan REO/t ash
Elements Zone I Zone Ⅱ Zone 3 Ⅲ (t/yr) yuan per kg million yuan/yr Zone 1 Zone 2 Zone 3
89
Ho 126 639 140 905 435.0 393.6 2.02 1.13 0.70
Total 26764 140380 32554 199698 20776.2 38238.6 180.10 111.91 66.30
a
1424 2020 price: the price of light rare earths and heavy rare earths derived from China Northern Rare Earth (Group) High-Tech Co., Ltd
1425 (http://www.reht.com/h-nd-426.html) and China Southern Rare Earth Group Co., Ltd.
1426 (http://www.zgnfxt.com/n91/n277/n279/c10814/content.html).
1427
90
1428 5. Speciation of REY in coal ash
1430 The combustion of coal in a utility boiler can significantly alter the speciation of
1431 REY in coal. As reviewed in section 3.2, the speciation of REY in coal ash has been
1432 extensively studied by techniques at the bulk [16,108,230] and micro scales
1434 carbon are the main components comprising coal ash. REY have been found to be
1435 associated with these three main phases. Based on the REY chemistry, mineralogy,
1436 and physical distribution within fly ash, the speciation of REY in coal ash is classified
1437 as: amorphous glassy associations; discrete minerals, both the major REE-bearing
1438 minerals and trace associations in other minerals, or compounds; and organic
1439 associations (bound to unburned carbon). The third type seems to be elusive with only
1440 a few TEM cases study finding it as inclusions dispersed into the amorphous and
1441 graphitic carbons, so that more studies and evidences are needed to make it clear and
1443
91
1444
1445 Figure 14. The classification of REY speciation in coal ash.
1446
1448 Aluminosilicate glasses are the dominant phases in coal-derived Class F fly
1449 ashes. A number of studies have indicated that REY associated with glassy materials
1451 shown in Figure 15, correlation analysis of REY contents versus major elements
1452 contents in fly ashes found that REY showed a positive correlation to SiO2 and Al2O3.
1453 Sequential chemical extraction studies on coal fly ash samples from Southwestern
1454 China [27], Eastern United States [260], and northeast Spain [171] indicated that more
92
1455 than 70% of REY was hard to leach in various acid solutions and was considered to
1457
1458
1459 Figure 15. The relationship between the concentrations of REY and major
1461 [18,25,32,120,169,178,186,191,252,259,261].
1462
1463 Amorphous Si-Al glassy associations can be further divided into those having
1464 REY dispersed throughout the whole glass grains and individual REE-bearing phases
1465 that are closely bound with Si-Al glasses (Figure 14). Scale is a key parameter to
1466 discern these associations and various microscale techniques, including SEM-EDS,
1467 EPMA, TEM and the related techniques, SIMS, synchrotron-based micro XRF
1468 imaging and micro XANES, and among others are necessary for identifying these
1469 REY forms. REY dispersed throughout the aluminosilicate glass have been reported
1470 in several instrumental studies. Using Ce as a proxy for all of the REY, an EPMA
1471 study of REY-enriched Kentucky fly ashes by Hower et al. [238] was conducted, and
93
1472 the WDS mapping observed that REY was distributed throughout the glassy ash
1473 particles, such as Si-Al glassy cenospheres and frothy glassy particles. Note that at
1474 that scale, EPMA may not tell if the Ce was truly dispersed or in fine minerals. The
1475 distribution of REY in individual fly ash Si-Al glass grains were determined using the
1476 Stanford/USGS SHRIMP-RG ion microprobe [146]. The uniform distribution of REY
1477 in single aluminosilicate particles to that of bulk fly ash is indicative of REY
1478 partitioning into the aluminosilicate glasses. In a study by Stuckman et al. [232], a
1479 suite of four coal fly ash and three bottom ash samples derived from the Appalachian
1480 basin was studied by synchrotron micro-X-ray fluorescence and near-edge absorption
1481 spectroscopy (μ-XRF and μ-XANES). The μ-XRF mapping showed that REY were
1482 dispersed throughout the aluminosilicate glass in irregular shapes with large grain size
1483 (> 40 μm). In another XANES study [233], linear combination fits of bulk Y-XANES
1484 spectra of nine fly ashes from the central Appalachian basin, Illinois basin, and
1485 Powder River basin found that 22-76% of REE occur as Y-doped glass. After
1486 leaching these ash samples with 1M oxalic acid, the bulk ash fits were dominated
1488 The close association of REY mineral particles with glassy matrices is another
1489 common REY occurrence in fly ash. In the study of Liu et al. [230], REY-rich
1491 coal-derived fly ash, and the REE minerals were found to be totally encapsulated or at
1492 the edge of Si-Al glasses. In combination of SEM-EDS and LA-ICP-MS, Thompson
1493 et al. [237] observed that small grains (~10 μm) of monazite, zircon, and apatite were
94
1494 commonly embedded within Al-Si glassy cenospheres, Al-Si spheres, or other
1495 aluminosilicate glass forms and the particle size of these REY-bearing glassy phases
1496 was mostly in the range of 50-80 μm (Figure 16). Synchrotron micro-X-ray
1497 fluorescence and near-edge absorption spectroscopy (μ-XRF and μ-XANES) also
1498 provide direct evidences [218]. In their study, Ce hotspots, an area (4–30 μm) denoted
1499 by the yellow to red color on the maps representing high XRF signal intensity, were
1500 mostly found within glass phase (13 out of 19) in μ-XRF maps. In six of 13 Ce
1502 The co-localization of Ce with Si, Al, Ca, P, Ti, and Nd suggested that monazite is
1504 co-localized with a range of elements, including Si, P, Ca, Fe, and other REE by
1506 REY phosphates, REY oxides, or REY carbonate making up these Y hotspots.
1507
95
1508
1509 Figure 16. SEM-BSE images of REY-bearing minerals encapsulated within glassy
1510 particles in a fly ash from a pulverized coal power plant in Ohio, USA. After
1512
1513 The use of TEM and related techniques, such as SAED and EDS can provide
1514 insights into the glass-REY mineral associations. TEM studies of REY-rich Kentucky
1515 fly ash samples have revealed a variety of REY-bearing minerals and amorphous
1516 phases to be present within the ash [122,144,192,231,236]. For example, Hower et al.
1517 [122] found ~10 nm xenotime (YPO4) particles included within monazite in the
1518 ponded ash from the burning of eastern Kentucky coal; the composite mineral
1519 assembles are within glass. The nanosized REY phosphates within glass phase were
1520 further confirmed by X-ray pattern of the separated REE grain after FIB extraction.
96
1521 Figure 17 illustrates a STEM image of a REY rich region, EDS mapping showing the
1523
1524 Figure 17. Images showing how a scanning transmission electron microscope (STEM)
1525 worked on identifying the fine REY-bearing mineral grains with the aid of SEM-BSE
1526 techniques. (a) SEM-BSE identified the REY-rich area for preparing the TEM lamella
1527 (yellow box); (b) STEM image of the selected area extracted by FIB technique high
1528 angle annular dark field (HAADF) mode. After Hower et al. [231]. Reproduced with
1530 A mineralogic examination of Figure 17 particle is seen on Figure 18, where the
1531 lattice interlayer spacing and the diffraction pattern, as derived from FFT and SAED
97
1532 indicates a Ce orthophosphate monazite, with a monoclinic unit cell. In addition to
1533 monazite, xenotime, zircon, and among other, crichtonite-group minerals, possibly
1535 found within Si-Al glass in a stoker ash from the combustion of REY-rich coal
1536 (Figure 19) [25]. However, some REY-rich areas have no discernable minerals, as
1537 indicated by SAED or FFT imaging for the crystallinity [144]. This may indicate that
1538 REY disperse into the glassy structures. The restrictions of the current technique
1539 determine that it cannot detect exceptionally fine minerals, overlapped, and/or
1540 disparate mineral grain orientations if REY present as the complicated forms.
1541
98
1542
1543 Figure 18. (a) Low-magnification bright field TEM image from the region shown in
1544 Fig. 18; (b) REY-containing area indicated in a yellow box; (c) Lattice fringe
1545 interlayer spacings determined by FFT; (d) SAED quantification obtained from the
1546 same region. After Hower et al. [231]. Reproduced with permission from Elsevier
99
1547
1548 Figure 19. (A) TEM bright field image of a REE-bearing mineral, possibly davidite
1550 diffraction pattern from SAED. (B) Element maps of Al, Ti, and Fe. (C) Element maps
1551 of Al, La, and Ce. After Hower et al. [236]. Reproduced with permission from
1552 Elsevier
1553
1556 coal ash. While aluminosilicate glass is the main ash components, it can observe that
1557 some discrete REY-bearing minerals/compounds have no contact with the glass
1558 phases. In comparison to the amorphous glassy associations as noted above, discrete
1559 REY minerals or/and compounds are not exclusively enclosed within the glassy
100
1560 matrix of coal ash, showing certain independence from the glass phases (Figure
1561 20-21). Typical discrete REY phosphates, REY carbonates, REY oxides, REY
1562 silicates, REY sulfates, REY-bearing iron oxides, etc., have been observed in coal fly
1563 ashes. By using polarized reflected-light and oil-immersion optics, Figure 20 (A)
1564 shows a monazite grain in a Kentucky Fire Clay coal-derived fly ash, and Figure 20
1565 (B) illustrates a zircon (a potential Y source) grain in fly ash from Powder River Basin
1566 subbituminous coal-derived fly ash. These two large mineral particles might be
1567 extreme examples of the discrete mineral/compound associations, since most REY
1568 particles in ash are too small to be observed using fly ash petrographic methods.
1569 Figure 21 illustrates a EDS mapping result showing that discrete REY-bearing
1572 a coal fly ash from combustion of coal from a Ohio pulverized coal-fueled power
1573 plant. Discrete pure REY phosphates (∼30-μm size) and minor REY contained in
1574 lime have been observed in two US coal fly ashes (Liu et al., 2019).
1575
1576
101
1577 Figure 20. (A) Monazite (m) with glassy particles in an Eastern US bituminous
1578 coal-derived fly ash. (B) Zircon (z) in fly ash from Powder River Basin
1579 subbituminous coal-derived fly ash. Images from Hood et al. [192].
1581 Kentucky Center for Applied Energy Research and the American Coal Ash
1582 Association. Reproduced with permission from Coal Combustion and Gasification
1583 Products.
1584
1585
1586 Figure 21. (A) SEM-BSE image of a fly ash derived from an Ohio pulverized coal
1587 power plant. (B) Mineral phases of fly ash (segmented image) are Al/Si-rich particles
1588 (blue), Fe-oxide (red), rhabdophane/monazite (yellow)), and CaO-rich (pink). After
1591 important for evaluation of REE extraction efficiency and some synchrotron
1592 microscopy and spectroscopy may provide some important information in this aspect
1593 [145,232,233]. The LCF of bulk Y XANES spectroscopy of fly ash from three major
102
1594 coal basins of the U.S. suggest that bulk ash fits were comprised primarily of
1595 Y2 O3 (18% to 51%) and Y-doped glass (22% to 76%) [233]. While in another Y
1596 XANES study [145], no Y-doped glass was detected in the LCF results; instead
1597 REY oxides (35-55%), REY-bearing hematite (20−30%), and REY phosphates
1598 (20−25%) or apatite (20−35%) consisted of the REY species in fly ash. Both of
1599 the bulk Y studies only used Y-doped glass as reference compounds, meaning
1600 that REY species closely bound with glassy materials (e.g., encapsulation or
1601 embedding) may not be detected by the method. This may cause the different
1603 in the same fly ash from that of bulk XANES. In Liu et al.’s study [145], twelve Y
1604 hotspots with particle size from < 10 μm to 50 μm in fly ashes was fitted and the LCF
1605 results of Y μXANES showed that five of the hotspots were identified as REY oxides,
1606 three as REY phosphates (churchite/xneotime), one as REE in Ca-rich Si-Al glass,
1607 and the rest had no results because of indistinguishable LCF data profile. Taggart et al.
1608 [233] observed great variations in μXANES fits among Appalachian basin, Illinois
1609 basin, and Powder River basin ashes. Results from XANES at both bulk and
1610 micro scale can be informative for knowing the speciation of REY in fly ash
1611 and contribute to the confirmation of certain amounts of discrete REY minerals
1612 or compounds in fly ash but is still challenging to provide a complete and
103
1614 5.4. Associations with unburned carbon
1615 Unburned carbon in fly ash has been proved to be important trapper for many
1616 trace metals, such as Hg, As, Se, and among others [262,263]. In a recent study by
1617 Hower et al. [264], the froth flotation of fly ashes collected from one power plant
1618 burning Pennsylvanian-age Kentucky coal generates low density, C-rich particles. The
1619 concentration of REY in the carbon froth concentrate (512 ppm) is comparable to the
1620 feed ash (464 ppm), indicating that the fly ash carbon may host certain amounts of
1621 REY. TEM studies found that graphitic and fullerene-like carbons, often containing
1622 included/entrained nanoscale minerals and/or metals, occur in the fly ash resulting
1623 from the burning of bituminous coal [122,192,235,265]. In accordance with the
1624 established occurrences of trace metals with fly ash carbon deposited on
1625 aluminosilicate glass particles, Hower et al. [122] and Hood et al. [192] observed
1626 association of REY with the nanosized carbons by HR-TEM technique. In Hood et
1627 al.’s study [192], a thin-layer carbon shell containing Ce and Nd is noted (Figure 22).
1628 The nano-sized carbon deposits onto a Si-Al-O glassy sphere. Similarly, in another
1629 study by Hower et al. [122], an complex ash constituent of Al-Si spheres, Fe-bearing
1630 minerals, and unburned carbon can be seen; the Al-Si glass sphere with an Fe-O core,
1632 The original construction implied that the REY are part of the graphite structure.
1633 However, the TEM resolution is still insufficient to distinguish if REY are in the same
1635 detailed view of the graphitic carbon at the scale of 10-nm including few-nano-size
104
1636 Ce and Fe particles [235]. The sample is a C-rich concentrate product produced by the
1637 froth flotation of a fly ash. Note that the locations of the Ce Lβ peaks are close to that
1638 of the La, Pr, Sm, and Gd peaks, which cannot be discerned by the software. It is
1639 suggested that these REY might also be present in the particles [235].
1640
1641
1642 Figure 22. HR-TEM image (upper left) of Al-Si glass sphere surrounded by graphitic
1643 carbon deposits, as indicated by EDS mapping of C, Nd, and Ce in the upper right,
1644 lower left, and lower right images, respectively. The fly ash is from the combustion of
1647 Kentucky Center for Applied Energy Research and the American Coal Ash
1648 Association. Reproduced with permission from Coal Combustion and Gasification
1649 Products.
1650
105
1651
1652 Figure 23. HR-TEM image (right) of Al-Si glass sphere surrounded by graphitic
1653 carbon deposits. The composite of 50 EDS scans (left) finds that the carbon contains
1657 Kentucky Center for Applied Energy Research and the American Coal Ash
1658 Association. Reproduced with permission from Coal Combustion and Gasification
1659 Products.
1660
1661
106
1662 Figure 24. (A) HR-TEM image of a graphitic carbon contains Ce and Fe (yellow box),
1663 as indicated by EDS spectra (B). Images from Hower et al. [122].
1665 Kentucky Center for Applied Energy Research and the American Coal Ash
1666 Association. Reproduced with permission from Coal Combustion and Gasification
1667 Products.
1668
1669 In addition to the association of metals with carbon surrounding Si-Al glassy ash
1670 particles, fly ash carbon also encases the Fe-spinels along with rare earth elements.
1671 Figure 25 illustrates the carbon deposit on the surface of the several spinel grains
1672 entraining Nd, Ce, Sm, and Y. The ash sample is a magnetic fraction of a beneficiated
1673 fly ash [192]. TEM imaging and the EDS mapping of the Fe-spinel minerals at a
1674 larger magnification further indicated that the spinel minerals occur in association
1675 with REY (Figure 26). The enrichment of some REY, for example Gd and Pr has
1676 been noted in the magnetic fractions of fly ashes from Eastern Kentucky power plants
1677 [12,122]. In their study [12], despite that the total REY contents of the magnetic
1678 concentrate (327 μg g-1) being lower than the clean product fraction (< 200 mesh, 485
1679 μg g-1), the Gd content shows a enrichment trend in the magnetic fraction (55 μg g-1
1680 for the magnetic fraction versus 18 μg g-1 REY for the <200-mesh fraction).
1681 Praseodymium is another element with a notably increased content in the magnetic
1683
107
1684
1685 Figure 25. HR-TEM image of spinel (sp) surrounded by an amorphous carbon with
1686 Ce, Nd, Sm, and Y-bearing inclusions. The area scanned by EDS is shown by the
1687 rectangle on the lower right. The fly ash is a magnetic fraction of a fly ash from the
1688 combustion of an Eastern US bituminous coal. Images from Hower et al. [122].
1690 Kentucky Center for Applied Energy Research and the American Coal Ash
1691 Association. Reproduced with permission from Coal Combustion and Gasification
1692 Products.
1693
1694 Overall, results of the TEM combined with the EDS mapping indicated that
1695 nanosized particles containing a broad suite of REY were found in amorphous and
1696 graphitic carbons surrounding and binding either aluminosilicate glass or iron spinel
1697 grains in coal ash. It seems that REY occurs as sub-micron, nano-scale mineral grains
1698 associated with fly ash carbons. In another sample from the study of Hower et al [122],
1699 some Ce oxide was observed as 1-2-nm spheres encased with carbon, suggesting that
1700 the particles may be formed in the ash by nucleation and growth, consistent with the
108
1701 observation of REY inclusions in graphitic carbons, which might form during
1702 incomplete combustion processes, not as the fractured remnants of minerals from the
1703 coal. However, unlike the REY minerals seen in the fly ashes, the association of REY
1704 with unburned carbon is very difficult to resolve and the formation mechanisms seem
1705 to be elusive. In contrast the visible individual mineral inclusions in the carbons, some
1706 REY either dispersed throughout (Figure 22) or incorporated into the fly ash carbons
1707 (Figure 24) are too small to be detected as independent mineral grains or really bound
1708 to the unburned carbon (like Hg-C structure). More research and evidence are needed
1709 for confirming those associations and the formation mechanisms in the future.
1710
1711
1712 Figure 26. (A) TEM imaging of Fe-spinel minerals (sp) in fly ash from the
1713 combustion of an Eastern US bituminous coal blend. (B) Composite EDS image
109
1714 based on the elements mapped individually in (C). Unpublished images from Hower
1716 University of Kentucky Center for Applied Energy Research and the American Coal
1717 Ash Association. Reproduced with permission from Coal Combustion and
1719
1722 When considering the fate of REY in coal-fired power plants, it is important to
1723 estimate the distribution of REY in various product streams. This determines which
1724 types of coal combustion byproducts are suitable for REY recovery upon the coal
1725 combustion. Generally, inputs of REY into a utility combustion system include coal
1726 and any additives, such as limestone for desulphurization, and urea for denitrification;
1727 the outputs from a coal-fired power plant include bottom ash, fly ash, gypsum, filter
1728 sludge, flue gas, and escaped fine particulate matter [266].
1730 Table 16 gives a summary of the distribution of REY among different emission
1731 streams of industrial coal-fired power plants. Several filed measurements and
1732 laboratory combustion tests estimated the overall mass balance of REY in various
1733 streams, finding the mass balance ratios greatly varied in different plants. In a work
1734 by Wu et al. [180], the distribution of REY in four China coal-fired power plants was
1735 investigated. The mass balance obtained for a 300-MW circulated fluidized bed boiler
110
1736 (CFB) and a pulverized coal-fired (PC) power plant were satisfied (79.4-103.4%).
1737 Only 37-79.4% REY recovery were obtained for another two power plants. In another
1739 behavior during coal combustion was performed at three pilot-scale combustion tests
1740 on a 50-kW underfed stoker unit. Good mass balance closures (81-84%) were
1741 achieved for REY (taking Ce as proxy) of the two combustion runs, with another one
1743 The mass balance ratio of REY by measuring the REY content in all types of
1744 solid products (e.g., gypsum) and particularly flue gas has rarely been reported. Based
1745 on US Environmental Protection Agency Method 29 (EPA Method 29) for sampling
1746 and determination of trace metals in flue gas , recent field measurements on five
1747 Guizhou coal-fired power plants in Southwest China indicated that the concentration
1748 of REY in gypsums and flue gases was low, with ranges of 5.7-11.7 μg g-1 and
1749 5.9-21.4 μg m-3, respectively [28]. The balance ratio for REY in the five power plants
1750 was acceptable (90.3-113.7%). Overall, a closed balance for REY in coal power plants
1751 is difficult to obtain and the evaluated ratios are subject to large errors. The lower
1752 mass balance ratios for some measurements may arise because (1) the collected
1753 combustion byproducts do not correspond the coal burned in the furnace, this usually
1754 occurs in utility boiler experiencing large deviations, such as the boiler load,
1755 combustion temperature, residence time, varying feed coal sources, and among others;
1756 (2) REY emitted as gaseous species are not determined; and (3) contaminants in
111
1758 Table 16. The distribution of REY across the whole power plants.
Boiler type Solid fuel Adsorbents Bottom ash fly ash Gypsum Stack gas References
Fuel property % Con Type Conc Conc f Conc f Conc f Conc μ f Balance
μg g-1 μg g-1 μg g % μg g-1 % μg g-1 % g m-3 % %
-1
1759 Conc: REY concentrations; f: mass fractions of REY in the combustion byproducts; r: as-received basis; ad: dry-basis.
112
1760
1762 Following the summary of Smith [267], Meij [266], and Clarke [268], and
1763 modified from Hower et al. [262], three groups of elements are broadly classified
1764 according to their volatility and partitioning behavior during coal combustion (Figure
1765 27). Due to the high boiling temperature, REY in coal are hardly volatilized and can
1766 be categorized as non-volatile elements. As shown in Table 16, almost all of REY
1767 partitioned into the solid ash after coal combustion. The mass fractions of REY in
1768 gypsum plus flue gas were calculated to be less than 1% [28]. Therefore, coal ash has
1769 been regarded as a primary byproduct for REY recovery. Moreover, it seems that fly
1770 ash may have more advantages for REY recovery than bottom ash in terms of the
1771 REY concentration and “reserve”. Mardon and Hower [250] arranged a set of
1772 REE-rich Fire Clay coals from a single seam of a single mine burned in a 220-MW
1773 wall-fired boiler for tracking the fate of trace elements in coal combustion. Fly ashes
1774 collected from the economizer, mechanical hopper, and electrostatic precipitator
1775 hopper have higher REY contents (average value of 1422 μg g-1, ash-basis) than
1776 bottom ash (1203 μg g-1, ash-basis). The slight higher REY contents in fly ash than
1777 bottom ash were also reported in many other power plants [24,27,119,161,178] . The
1778 mass ratio of fly ash to bottom ash for utility PC boilers varied significantly, but
1779 generally around 4:1. As a result, during coal combustion, most of REY in coal could
1780 transfer into the fly ash. In the studies of Wu et al. [180] and Li et al. [28], REY in
1781 coal fly ash derived from nine Chinese power plants show higher mass ratio of 42-94%
113
1782 than that of bottom ash (6-58%) [28,180]. These results could be useful for selecting
1783 REY sources from coal combustion byproducts. Note that an uneven distribution
1784 between fly ash and bottom ash does not follow the classification of trace element in
1785 Figure 27 [266]. The variation of REY contents in fly ash as a function of particle
1786 sizes and collection arrays in power plants is not only controlled by the REY volatility
1788
1789
1790 Figure 27. Distribution of elements among bottom ash, fly ash, and flue gas. After
1791 Hower et al [262]. Reproduced with permission from Elsevier. Boiling points after
1792 Wang et al.[269]. This is a generalized concept and actual performance in pollution
1793 control systems may vary. The elements emphasized in this paper are shown in bold
1794 italics.
1795
114
1796 6.2. REY partitioning within ash-collection systems
1798 The distribution of REY content within fly ash collection system, i.e.,
1799 electrostatic precipitator (ESP), baghouse or fabric filter (FF) is firstly dependent on
1800 their concentrations in feed coal. After coal combustion, the partitioning of several
1801 volatile elements (Group 2&3 in Figure 27) within ESP or FF is a function of flue gas
1802 temperature and particle size at the collection point [272] . As with the decreased flue
1803 gas temperature and ash particle size, the concentration of volatile trace elements
1804 trend towards the back row of the ash collection system. Unlike the volatile trace
1805 elements (e.g., Hg, As, and Se), rare earth elements have very low volatility; therefore,
1806 significant variations in REY content may not be expected among the fly ashes
1807 collected from different zones of individual fly ash collection systems. The study of
1809 mechanical (cyclone)/three-row ESP ash collection system is a good case showing the
1810 REY distribution in fly ash capture system [250]. The fractionation of REY in the
1811 mechanical and ESP fly ashes, while variable, shows less temperature-related
1812 distribution than observed in the volatile elements. Rather, the total REY fall within a
1813 narrow range of 1214-1668 μg g-1 (Figure 28 (a)). A decrease in the ratio of LREE
1814 (La through Eu) to HREE (HREE: Gd through Lu) can be observed from mechanical
1815 rows (> 8) through the last row of ESP (< 6) (Figure 28 (b)). Hower et al. [167] also
1816 noted the fractionation between LREE and HREE after examining the chemistry of
1817 paired feed coal and corresponding ash from five different anthracite-burning stoker
115
1818 boilers. Light lanthanides decreased in concentration relative to heavy REE, as seen in
1819 the average coal LREE/HREE (9.8) against the average ash LREE/HREE (9.4). The
1820 decrease in the average Ce /Ce∗ (3.7 to 3.4) while increase in Gd /Gd∗ (1.9 to 2.1)
1821 from coal to ash also indicates a shift in LREE and HREE during coal combustion.
1822
1823
1824 Figure 28. (a) Variation of REY in fly ashes at different collection points of the ash
1825 collection system. (b) Variation of light REE to heavy REE ratio in fly ashes at
1826 different collection points of the ash collection system. Mech-1: 1st -row mechanical
1827 hopper ash; Mech-2: 2nd -row mechanical hopper ash; ESP-1: 1st row ESP ash; ESP-2:
1828 2nd -row ESP ash; ESP-3: 3rd -row ESP ash. Data was compiled from Hower et al
1829 [250,262].
1830
1831 Similar to the REY variation in the study of Hower [250,262], the enrichment of
1832 heavy lanthanides towards the back rows of the ash collection systems is notable in
1833 another three Kentucky power plants plus power plants from Bulgaria [259]. There
1834 are three- to five-row mechanical/ESP-ash collection system installed within these
1835 power plants, burning coals of varying ranks (lignite, subbituminous coal, and
116
1836 bituminous coal), with Plant P exclusively burning a small amount of waste tires with
1837 high-S coal. When the last-row ESP lanthanides are normalized to the first-row REY
1838 concentrations, all cases exhibit an enrichment in the HREE (Figure 29, after Hower
1839 et al. [259]). The ratio of critical to total REY also increases from the front ESP rows
1841 Overall, there is no significant partitioning of REY within ash collection systems.
1842 Nonetheless, with respect to the enrichment of HREE in coal fly ash especially the
1843 back rows of ash collection system, the detailed mechanisms are still not well
1844 understood. It is known that the flue gas temperature and particle size decrease with
1845 increased distance from the boiler. In the study of Liu et al. [158], the distribution of
1846 REY in a series of fly ash derived from the combustion of coal at a 100-MW
1847 pulverized-coal-fired power plant in southeastern Kentucky was measured. The ratio
1849 the last row of ESP (4.74), suggesting the enrichment of HREE would be associated
1850 with either a decrease in flue gas temperature or in the fly ash particle size. Fly ash
1851 petrology may provide some evidences explaining the increased HREE contents in
1852 fine fly ash, which might be due to [262] (1) the result of HREE having an affiliation
1853 to the organics in feed coal; and (2) the capture of the fine REY minerals into the
1854 glassy particles varying in size, chemistry, and structure, demonstrated by fly ash
1855 petrology study of sized fly ash, which will be discussed below.
1856
117
1857
1858 Figure 29. The normalization of REY contents in the last row ash to the first-row
1860
1861 6.2.2. Variations of REY in sized fly ash and implications for REY partitioning
1862 trend
1863 The particle size distribution of REY in fly ash is important to REY beneficiation
1864 from bulk ash into sized ash containing high contents of REY [21,166,259]. To
1865 understand the variation of REY contents versus particle size, the size dependence of
1868 500-mesh), the REY concentrations in sized fly ash (100-500 mesh) of individual
1869 hoppers, as examined by Liu et al. [158] noted above, have no defined trend (Figure
1870 30a). For the fly ash with particle size lower than 200-mesh size, the ratio of
118
1871 LREE/HREE decreases with the decrease in ash size for all the ash hoppers (Figure
1872 30a). Similar to Liu et al. (2014), the enrichment of REY and decrease in
1873 LREE/HREE in the finest fly ash by sieving is also reported by several investigations
1874 [21,23,167,192]. However, one exception study of the sized fly ash from Jungar
1875 power plant found that the concentration of REY in the finer fly ash were not
1876 significantly enriched and only increased by a factor of less than 2.5. For fly ash with
1877 much smaller particle size (< 20 μm), the enrichment of REY in the finer sized ash
1878 was noted in two cases study [166,170]. With an air-based classifier, fly ash was
1879 separated into size down to 2.2 μm (the whole size ranging from 2.2 to 43.2 μm), and
1880 REY exhibited an increase in the finest size fraction but depleted in the second-finest
1881 sized ash (2.2-9.7μm) relative to the bulk fly ash [166]. In another study [170], fly ash
1882 was separated into 0.3-2.5 and 2.5-10 μm size range using a cascade impactor. The
1883 contents of REY increased from 352.4 µg g-1 in the fine fly ash (2.5 -10 μm) to 384 µg
1885
1886
119
1887 Figure 30. (a) Variations of REY contents and LREE/HREE in size fractions of
1888 each of the ash collection systems in a U.S. Kentucky power plant [158,259].
1890 hopper ash from Jungar power plant, Inner Mongolia, China [24].
1891
1892 Overall, as non-volatile elements, REY show an enrichment in finer fly ash but a
1893 relatively random distribution in the whole size range, and the enrichment of HREY
1894 (decreasing LREE/HREE) towards the finer fly ash is notable. The normalized
1895 distribution pattern of REY versus the particle size provides clues for REY partition
1896 among various sized ash (Figure 31). Here, the sized ash from the same hoppers from
1897 a southern Kentucky power plant perhaps gives the best examples, since coal feed to
1898 the boiler was specially arranged from a single coal seam from a single mine, thus
1899 eliminating the variations from multiple coal sources on REY fractionation during
1900 coal combustion [158,250]. As shown in Figure 31, all sized fractions show similar
1901 distribution pattern, characterized by medium REY enrichment mode and positive
1902 anomalies of Eu and Gd. This suggested that there is no notable fractionation among
1903 different size fractions. Difference in fly ash petrology may account for the
1904 LREE/HREE distributions. For the two most abundant fractions of mechanical ash,
1905 LREE/HREE significantly differs between the 100-325 mesh ash (7.30-7.37) and the
1906 fraction < 325 mesh (5.35-5.94). The 100-325 mesh ash has 70.1% glass compared to
1907 85.8% glass in the <325-mesh fraction. As summarized in section 5, REY bound with
1908 glassy materials is the dominant association in coal fly ash. Variations in the amount
120
1909 and size of REY minerals between and in the microscopically identifiable fly ash
1910 constituents can contribute to the differences in REY contents across the
1912
1913
1914 Figure 31. The normalized REY distribution pattern (relative to REY in UCC) in
1915 fly ash from the same hopper in a southern Kentucky power plant: (a) different size
1916 fractions of fly ash from the economizer hopper and (b) different size fractions of fly
1917 ash from the mechanical hopper. Data was compiled from Liu et al. [158] and Hower
1919
1922 Phosphate minerals such as monazite and xenotime are the common
1923 REY-bearing minerals found in coal (see section 2.3). These phosphate minerals have
1924 high melting temperature point, depending upon their elemental components:
1928 remain intact during coal combustion and, after removal of organic matter, should be
1929 more commonly seen in coal fly ash than that in the feed coal. However, the
1930 mineralogy study of fly ash at micro-scale does not support this deduction. The
1931 microanalysis of REY-rich coal, for example, the well-known REY-bearing Fire Clay
1932 coal [36,46,135], can readily find discrete monazite particles and other REY-bearing
1933 minerals (such as zircon) at several microns disseminated through the coal matrix. In
1934 contrast, the fly ash has few REY mineral grains that can be seen by optical/electron
1936 scarcely to be observed at the scale of optical/electron microscopy, where are the rare
1937 earth elements in fly ashes? Hood et al. [192] demonstrated that pure monazite grains
1938 (hundreds of micrometers) will shatter into micron and sub-micron particle at 1400 ºC
238 232
1940 expansion of He produced from the decay of U and Th [274–276]. Among the
1941 other important REY minerals in coal, REE-bearing carbonates may also experience
1942 fragmentation at boiler temperature because the release of carbon dioxide [230].
1943 Zircon will decompose to zirconia and cristobalite in the temperature range of
1944 1285-1720 ° C [277]. Apatite, fluorapatite, and zircon may also experience
1946 REY-bearing CaO, and other unknown phases at a few μm to nm are observed in fly
1947 ash, suggesting the REY mineral fragmentation contributes to the final distribution
122
1949
1950
1951 Figure. 32 (A) Original pure monazites observed under optical microscopy. (B)
1952 Monazite after heating to 1400 ℃ observed under optical microscopy. Images from
1954 University of Kentucky Center for Applied Energy Research and the American Coal
1955 Ash Association. Reproduced with permission from Coal Combustion and
1957
1959 While the REY minerals are thermally stable, REE-bearing phases in coal may
1961 example, the XANES results of Ce in fly ash samples have identified that the
1962 redox-sensitive trivalent REE (Ce) could be changed into high valence state (RE4+)
1964 in coal can provide insights into the transformation behavior of REE during coal
1965 combustion. Liu et al. [230] used an in-situ XRD combined with a thermal analyzer to
123
1966 monitor the phase transformation of typical pure REY phases at the temperature range
1967 of 25-1000°C (Figure 33) and found that (1) REE-organic compounds and REE
1968 carbonates will decompose (T > 300 ℃) into oxides; (2) water-bearing REE
1969 phosphates will lose water after heating with no Ce oxidation; (3) REE phosphates
1970 such as monazite and xenotime have no structure change; but (4) REE-bearing
1971 phosphates (e.g. apatite) and zircon show characteristics of melting on mineral surface.
1972 A summary of the thermal conversion pathways of typical REE forms in coal is
1974
1975
1976 Figure 33. Thermal decomposition curve of individual pure REE-bearing phases at
1977 the temperature range of 25-1500 ℃ via thermogravimetric analysis under air
1978 atmosphere. After Liu et al. [230]. Reproduced with permission from Elsevier.
1979
124
1980
1981 Note that the combustion temperature (< 1000 ℃) of the experimental devices
1982 limits Liu et al’s [230] observations and conclusions. First of all, the flame
1983 temperature for the most-commonly used pulverized coal-fired boiler varies from
1984 1200-1800 ℃. When the combustion temperature is above 1000 ℃, the stable REE
1985 mineral phases may shatter into small grains (such as monazite) or chemically
1986 decompose into other phases (such as zircon), as mentioned above. In addition, as an
1987 important carrier for REY in coal, apatite is not stable and can transform into other
1988 phases with temperature being greater than 1000 ℃; and the decomposition
1989 temperature is dependent on the anion position in the hexagonal axis showing
1991 (Table 17). Secondly, there are still many of other REE minerals or non-mineral
1992 phases, such as REY carbonates (kimuratie and lanthanite) and REE-bearing clay
1993 phases requiring an in-depth study for their combustion behavior. As noted in 2.3,
1994 most of REE mineral grains are included within coal macerals, thus the combustion
1995 atmosphere (reducing or oxidizing) should be considered in the future work for a
1998
2000 common REE-phases during coal combustion. Compiled from Liu et al. [230], Hood
125
REY speciation Thermal conversion pathways
compound state
associations (Ⅳ)
(Ⅳ)
(Ⅳ)
(Ⅳ)
ºC; oxidation
Chlorapatite structure
at 1530 ºC;
Hydroxyapatite
126
1285 ºC)
2002
2003 After coal burning, fly ash will be exposed to flue gas with varying temperature
2004 along the process path from the flame zone (1300 -1700 ºC) to the inlet of ESP or FF
2005 (around 150 ºC). Flue gas is a complicated oxidizing system, in which the gas
2006 compositions mainly consist of N2, CO2, H2O, and O2; minor amounts of NOX, SOX,
2007 CO, HCl, and Cl2; and trace amounts of gaseous heavy metals such as Hg [279–281].
2008 In the complex environment of flue gas, the REY associations contained within fly
2009 ash could be impacted due to the reactions occurring between fly ash and flue gas.
2010 There are about 30s are available for the occurrences of the gas-solid reactions [282].
2011 A good example of the reactions between flue gas components and REY speciation
2012 can be the presence of Ce (IV) in coal ash, despite that Ce (III) might be the dominant
2013 valence state (> 85%) in coal-derived fly ash [230,232]. Using the µ-XRF mapping
2014 and μ-XANES techniques, Stuckman et al. [232] observed the co-existence of Ce, S, P,
2015 and Ca in eleven coal ash samples, inferring the formation of REE species such as
2016 REE-bearing sulfates and carbonates in the transport process of coal-derived flue gas
2017 in power plants. Bulk Ce XANES spectra of some fly ash samples also matched the
2018 reference Ce (III) chloride spectra, suggesting a chlorination of REY in the flue gas.
2019 In another study by Taggart et al. [233], bulk Y XANES results indicated that Y
2020 coordination states in class F fly ash samples resemble a combination of Y-bearing
2021 carbonates and other species (Y-doped glass and YPO4); whereas Y spectra of class C
127
2022 fly ash shows characteristics of Y2(SO4)3. Potential reactions of REY species in fly
2023 ash with flue gas components can be described as following [42,253]:
2027 (6)
2029 Apart from organic-bound REY, REY in coal is seldom vaporized into gaseous
2030 form in flue gas during coal combustion [230,251]. Most of REY in coal is
2031 transformed into the solid residual (mainly fly ash) (Table 16). As discussed in
2032 section 5, the instrumental analysis and chemical leaching of REY from coal fly ash
2033 demonstrated that a large fraction of REY is captured and enclosed within the
2034 Si-Al-based glassy materials. This would be understandable since the glass is usually
2035 the most abundant constituent in coal ash [283–285]. However, the detailed retention
2036 mechanisms are unclear. This is largely because (1) the details of the decomposition
2037 and chemical reactions of various coal minerals in combustion process, especially for
2038 a particle containing a mixture of mineral inclusions are poorly understood [160]; and
2039 (2) the morphology, chemistry, structure, and size of glass in coal ash itself are
2040 complex to be characterized [286,287], which will influence the reactivity of fly ash
2041 glass [288–291]. The fly ash glass reactivity is important in many areas, for example
2042 the use of fly ash as a pozzolan in concrete [292,293], the environmental leachability
2043 of hazardous elements released from ash landfilling sites [286,290,294], and the
128
2044 recovery of valuable metals as we discussed in this study. Therefore, the following
2045 section will make a short review on the characteristics of fly ash glass, providing a
2046 basis for understanding the close association of REY with glass and for designing an
2050 formed upon the melts cooling. Glass is also regarded as a super-cooled liquid product
2051 obtained from high-temperature melt [296]. From the point of mineralogy and
2052 petrology, fly ash is essentially composed of crystalline minerals, unburnt carbon, and
2053 non-crystalline aluminosilicate glass [297]. For coal ash, quantitative X-ray
2054 diffraction researches [285] and petrographic examinations [297–299] indicate that
2055 the Si-Al glass is the dominant phases in most fly ashes; and it is not a uniform and
2058 oil-immersion optics [300,301], with the unburned carbon usually being the main
2059 target [296,337, 340],[300]. In the case of inorganic compositions of coal ash, Hower
2061 components as amorphous glass, mullite, crystalline silicates, spinel, lime, sulfates,
2062 and oxidized minerals (Figure 34). Under optical microscopy, typical fly ash glass
2063 includes: amorphous solid and frothy phases (Figure 35A), glassy cenospheres
2064 (Figure 35B), and pleiopheres (Figure 35B). The formation of these different glasses
129
2065 in the context of pulverized coal-fired (PC) combustion involves the mineral reactions
2066 in the melting and cooling history of coal ash, which can be summarized as:
2068 clays) in combustion zone to mullite, spinel, cristobalite and liquid phase, which
2070 melting of the mineral products to liquid droplets on the surface of the coal
2071 particle and coalescence into large particle as the char burning [287,303–305];
2072 and
2074
2075
2076 Figure 34. Basic nomenclature of fly ash components based on the optical
2078
130
2079 Feed coal mineral types and temperature are important factors affecting the
2081 [287,297,302,303,305,306]. Clay minerals usually dominate the coal mineralogy and
2082 are the main sources for silicate melts and glass formation. The combustion behavior
2083 of clays and other common minerals including quartz, carbonates, and pyrite in coal
2085 minerals and their decomposition products having high melting point above the boiler
2086 temperature include: (1) crystalline minerals including quartz, mullite, lime, MgO,
2087 etc., and (2) poorly-crystalline materials such as cristobalite. These minerals and their
2088 intermedia products may survive the whole coal combustion process.
2089
2090
2091 Figure 35. Inorganic components of coal fly ash observed by optical microscopy
2092 under polarized light. A: Solid (s) glass spheres. B: Glass cenospheres (c) and
2093 pleiospheres (p). C: Mullite (m). D: Needle-like spinel — magnetite plus Cr, Ni,
2094 Al-spinels. E: Spinel in a sphere. F: Quartz (q). Basic nomenclature of fly ash
131
2095 components based on the optical petrology method. Field of view about 220 μm on
2096 long axis. After Hower et al. [299]. Reproduced with permission from Elsevier.
2097
2098 Table 18. Generalized scheme of behavior of common coal minerals during
2099 combustion and boiling points of the combustion products. After Hower et al. [297].
Mineral matter Combustion process and combustion products Melting points (℃)
Mullite:1850 ℃
Dehydration and sintering; possible mullite; reactions of
K/Na/Ca Feldspar:
Clays products with Fe2O3 from pyrite; CaO from carbonates, SiO2,
1100-1550 ℃
etc.to form glass or minerals
Quartz: 1750 ℃
Relict; reaction with aluminosilicates from clays, with CaO Na-silicate: 1089 ℃
Quartz
and Fe2O3 to form crystalline and molten silicate phases Ca-silicate: 1540 ℃
2100
2101 However, note that the melting point of a mineral may change, largely depending
2102 upon the mineral compositions, mineral-mineral association and the combustion
132
2103 atmosphere (oxidizing or reducing). For example, the clay mineral decomposition
2104 products typically melt at above 1400 ℃, but the melting can occur at around 980 ℃
2105 for SiO2-Al2O3-K2O eutectics. This is often seen in illite and smecite combustion
2106 process, which have certain amounts of alkaline elements [308]. Besides, the
2107 “included” clay minerals usually co-exist with other minerals within individual coal
2108 particles [310,311]. Table 19 gives the types of mineral-mineral association in a U.K.
2109 bituminous coal as determined by CCSEM technique [310]. As expected, clays are the
2110 dominant associations and almost 40% of the mineral matter are present as multiple
2111 mineral occurrences in a single coal particle. Thus, the mineral reactions in coal
2112 burning are not only self-transformations but thermal reactions of their intermediate
2113 products with other minerals and mineraloids. Melting of the thermal inactive
2114 components (quartz and clay decomposition products) with adding modifiers may
2115 occur as the burnout of coal particles (mineral coalescence) [287,305,310,312]. For
2116 example, the SiO2-Al2O3-CaO system has several eutectics at around 1200-1300 ℃
2117 [313–315]. At 1000-1200 ℃, pyrites co-existing with clay minerals in a single coal
2118 particle (reducing atmosphere) have preference to coalesce with their intermedia
2120 SiO2-Al2O3-FeO-K2O liquid system [308,313,316,317]. This process may also have
2121 influence on the REY mineral transformation, as will be discussed in next section.
2122
133
2123 Table 19. Quantification of mineral-mineral associations in a pulverized bituminous
2124 coal fed into U.K. power plants by the means of CCSEM. Data from Wigley and
clay 37.1
Pyrite 7.8
Quartz 3.8
Fe-clay 3.3
Accessory 2.4
Calcite 2.1
Other 8.1
2126
2127 To summarize, the melting of inorganic components in boiler is the basis for
2128 glass formation in fly ash. When the coal particles burn in a PC boiler, spherical
2129 droplets and inflated molten particles derived from the combustion of clay and other
134
2130 minerals suspended in the combustion zone are the two notable features. As the
2131 particle leave the boiler, the quenching of the spherical molten particles will form the
2132 spherical glassy particle. If the included minerals within coal particles are fully melted,
2133 the gases released from the decomposition of char, carbonates, sulfide minerals, and
2134 vaporization of pore water may be trapped in the liquid microspheres. Then the gases
2135 can bloat the molten melt up to a 500-μm diameter hollow particle [303,318,319]; and
2136 the size and the thickness of the particle (cenosphere) are a function of the melt
2137 viscosity and gas pressure. The pure mineral decomposition and reactions are
2138 important to understand the formation of silicate liquid but cannot capture the real
2139 interactions among two or more different minerals in coal combustion process. The
2140 details of the mineral-mineral reactions, especially for a mineral mixture containing
2141 one or more types of mineral inclusions are poorly understood [302,306,310,320,321].
2142 Besides, fly ash glass usually co-exist with crystalline minerals, for example
2143 magnetite and mullite crystals presenting as a spherical shell of the fly ash glass
2144 [286,299,302]. These minerals are derived from either recrystallization of the melts or
2145 directly from parent mineral transformations in the thermal conversion process
2146 [302,306,322]. The REY phases that are immediately adjacent to or surrounded by the
2147 mineral phases (such as mullite and quartz) within a dense Al-Si glass would offer
2148 physical resistance to the release of REY from fly ash [122,144,231].
2151 solids [296]. These terms are considered to be synonymous, revealing the state of
135
2152 atoms in the glasses are highly disordered. For fly ash glass, it mainly consists of
2153 silicate and/or aluminosilicate glass, and it can be simply described as“… an
2154 inorganic product of fusion which has been cooled to a rigid condition without
2155 crystallizing.” [323]. Many attempts have been made to understand the structure of
2156 silicate melts and glass materials. It is beyond the scope of this study to review the
2157 extensive papers on glass structure and its formation mechanisms, but generally, the
2158 random network model and crystallite model can be used as two typical models for
2159 the description of silicate glass structure [323]. For a complex system such as coal fly
2160 ash, the random network model proposed by Zachariasen [324] that was established
2161 on the basis of crystal chemistry view of Goldschmidt has been widely used
2162 [287,290,291,298]. The glass structure in coal ash and its relationship with glass
2163 composition are very complex, because the inter- and intra-particle heterogeneity of
2164 fly ash brings difficulties to an absolute understanding of fly ash glass
2165 [287,288,290,305,306]. A basic knowledge is that the structure and chemistry of the
2166 fly ash glass vary with the feed coal properties and the boiler operational conditions.
2167 Structurally, the atoms in silicate glass are disordered arranged in long range but
2168 has short- and medium-range order. This short-range order but long-range disorder
2169 atomic model has been extensively examined by various analytical methods, for
2170 example extended X-ray-absorption fine structure, nuclear magnetic resonance, and
2171 nano-beam electron diffraction [325–331]. The structure disorder in fly ash glass has
2172 been considered as a result of three factors [284]: (1) rapid quenching of silicate melts;
2173 (2) network isomorphic substitution; and (3) cation modification. The tetrahedral
136
2174 [SiO4] is the skeleton of the fly ash glass according to the network theory [324].
2175 Usually, though, fly ash glass has a multi-component chemistry and is more complex
2176 than the vitreous SiO2. In the three-dimensional network structure, the co-melting of
2177 silicon oxides with other network formers such as Al3+, Fe3+, and Ti4+ (with
2179 introduction of network modifiers, such as Na+, K+, Ca2+, Fe2+, and Mg2+, with
2181 modification). The intermediates, such as Al, can either reinforce (coordination
2182 number of four) or weakens the network (coordination number of five or six),
2183 depending upon the amount of Al and the modifier elements [284,287,305,307].
2184 Accordingly, both of the substitution and cation modification order would prevail in
2185 the structure of fly ash glass [284,308]. For example, the position of 2θ in XRD
2186 patterns of sodium silicate shows a marked shift in the halo to a higher angle (32-34°)
2187 with increasing Na2O content (0-50%) [323]. In another study, Brindle and McCarthy
2188 [305] extensively examined the relationship between ash glass content and glass
2189 chemistry of 75 European fly ashes. Their result suggested a major influence of alkali
2191 The chemistry of fly ash glass is dominated by SiO2, Al2O3, CaO, and Fe2O3;
2192 with minor MgO, K2O, Na2O, P2O5; and trace elements including rare earth elements.
2193 Based on the structural characteristics of the major components, Hemmings and Berry
2194 [284] summarized that the chemistry of fly ash glass locates between silica fume and
137
2196 lignite ash bituminous ash has 72% network formers (SiO2 + Al2O3 + Fe2O3) and
2198 subbituminous ash has 81-84% network formers (SiO2 + Al2O3 + Fe2O3) and
2200 bituminous ash has 84-90% network formers (SiO2 + Al2O3 + Fe2O3) and 10-16%
2202 However, the result is a general summary of chemical compositions of fly ash
2203 glass. Ash particles may greatly vary in their compositions from grain-to-grain
2204 (inter-particle difference) in a fly ash derived from the burning of the same coal at a
2205 power plant. This extreme heterogeneity of fly ash is a result of (1) feed coal
2206 properties, i.e., variations in coal rank and seam to seam changes resulting in the coal
2207 mineralogy that are differentiated largely by the alkaline and alkaline earth element
2208 contents, e.g., lignite usually contains more of K, Na, and Ca than bituminous coal
2209 [283,312]; and (2) variations in the formation conditions and collection points at the
2210 power plants, for example, the boiler condition, load, ESP fields, and among others
2212 differences of REY among various glasses in coal ash due to its trace amount in coal
2213 ash.
2214 6.4.3. Possible incorporation mechanisms of REY into fly ash glass
2215 Based on the study of REY speciation in coal ash and the glass formation
2216 mechanisms during coal combustion, two capture mechanisms can be broadly
2217 proposed:
138
2218 the incorporation of individual fine REY-bearing mineral grain into Si-Al melts
2220 the incorporation of rare earth elements into the aluminosilicate glass structures in
2222 The first capture mechanism has been demonstrated by numerous electron
2224 grains such as monazite, xenotime, zircon, and apatite at varying size (from several
2225 microns to nanometers) are observed to be partly or fully embedded within fly ash
2227 factor influencing the process. As indicated in section 2.3, prior to combustion in
2228 coal-fired boilers, these REE-bearing minerals are almost dispersed within coal
2229 organic maceral as included minerals (Figure 6a and 6b); and usually intermixed
2230 with other major coal minerals (such as clay minerals in Figure 6c and 6d). In this
2231 case, incorporation of these REY-bearing mineral grains into glassy components can
2232 occur when the silicate melts form at PC boiler temperature (1300-1700 ℃). The
2233 stable REY mineral grains or its derivative products will naturally enclosed within the
2234 new-formed glass upon the cooling of the melts, at concentration and particle size
2235 usually below the detection limit of XRD and optical microscopy techniques,
2237 Another possible pathway for capturing the REY mineral inclusions may result
2238 from mineral collision and coalescence during the burnout of parent char particles
2239 [310]. Mineral coalescence has been used to describe the ash formation mechanism,
139
2240 and conditions for completing the mineral coalescence generally require [334]: (1) at
2241 least two mineral grains included within one coal particle, (2) the local temperature is
2242 enough for mineral melting, and (3) contact between the molten particles. As
2243 indicated in Table 19, individual coal particles often contain more than one mineral
2244 grains, where REY phases may be present in some coal particles. For PC boilers
2245 operating at normal temperature (> 1300 ℃), the included REY-bearing constituents
2246 and the melted silicates will be exposed as the decomposition and oxidation of coal
2247 char particles. The distance between the ash droplets and REY minerals decreases as
2248 the char combustion progress and finally would contact and merge into one large
2249 particle in case of no fragmentation. Due to thermal stability of REY minerals, the
2250 heterogeneity of the coalescent particles may exist, for example monazite and zircon
2251 still persist in the large cenosphere or solid glassy sphere particles after coalescence
2252 (Figure 16). Note that the coalescence of minerals is limited to the coal char
2253 fragmentation. If there is no char fragmentation, all the included minerals in a single
2254 coal particle can be merged into one large particle (full-coalescence) after the
2255 complete burnout of char [335,336]. But char fragmentation is usually seen in coal
2256 particle combustion which may diminish mineral coalescence [337,338]. A negative
2257 relationship between coal particle fragmentation and mineral coalescence can be
2259 partial-coalescence, and no-coalescence have been proposed for different scenarios of
2261 account for the REY associations in coal ash, that is, REY minerals are observed to
140
2262 have fully enclosed, partially enclosed, or have no contact with the glassy particles in
2263 coal ash. Besides char fragmentation, the extent of mineral coalescence is also
2264 influence by the boiler type, mineral types and associations, and mineral particle size
2265 [142].
2266 In the case of the second retention mechanism, although most of the
2267 REY-bearing phases in coal have high melting points, the incorporation of
2268 REY-bearing phases into silicate melts (co-melting) might occur if (1) the local
2269 temperature is high up to the melting interactions; (2) active components (e.g.,
2270 Na2O/CaO) exist in the silicate melts, and interactions between physically- associated
2271 minerals may be likely to bring about thermal chemical reactions at a high
2273 aluminosilicate glass particles via SHRIMP-RG analysis may support the REY
2274 incorporation mechanism [146]. The REE distribution patterns in different fly ash
2275 glasses, i.e., Al-rich aluminosilicates, Si-rich aluminosilicates, and Ca- and Fe-rich
2276 aluminosilicates, are similar to that of the bulk ash (Figure 36 a). As shown in Figure
2277 36 b, one zircon particle is found in the ash samples but the chondrite-normalized
2279 type) from the bulk fly ash (LREE-enrichment type). If the discrete mineral dominates
2280 the REY associations in ash, then the normalized distribution pattern cannot be
2281 consistent among various ash particles (see Figure 31 and 36a). Therefore, the
2282 enrichment of REY in coal ash would be explained by the diffusion of REY into the
2283 fly ash glass at the expenses of REE trace phases in coal [146].
141
2284
2285
2286 Figure 36. (a) Distribution pattern of REE in various aluminosilicate glass particles in
2287 a coal fly ash derived from the combustion of Power River Basin coal. (b)
2288 Distribution pattern of REE in zircon in different coal fly ashes from Jungar power
2289 plant in Inner Mongolia, China and from Central Appalachian Basin, eastern United
2290 States. Data was compiled from Kolker et al. [146] and Dai et al. [24].
2291
2292 The incorporation mechanisms are somewhat analogous to the process in making
2293 rare earth silicate glass and in natural igneous system [342,343]. The incorporation of
2294 rare earth oxides (RE2O3) into aluminosilicate glass usually occurs at around 1500 ℃
2295 (melting temperature) [344–352]. This suggest that similar processes may occur
2296 inside the pulverized coal-fired boilers, where the normal operating temperatures are
2297 maintained in 1300-1700 °C. On the basis of reactions for producing REY-bearing
2298 silicate glass, the REE trace phases, at least for some REY-bearing oxides generated
2300 dispersed into the silicate melts. Even for the thermal stable REE phosphates (such as
142
2301 monazite), potential reactions for decomposing monazite would happen when active
2305 significantly lower than the coal combustion temperature in power plants. Note that
2306 the reaction rate is limited by the solid diffusion rate; however, the multi-component
2307 coal-derived silicate melts (especially containing high amounts of network modifiers)
2308 would favor the reaction because the mass transfer process could be improved within
2310 Local structure of REY in the silicate glass network can provide more details
2311 about the REY incorporation mechanisms. Various techniques, for example magic
2312 angle spinning nuclear magnetic resonance spectroscopy, Raman spectroscopy, X-ray
2313 and neutron diffraction spectroscopy, X-ray absorption fine structure (XAFS), and
2314 atomistic molecular dynamics simulations have been used to understand the structure
2316 in a Y-bearing glass model complexes [348] (Figure 37), the primary units of the
2317 network are basically composed of SiO4 and AlO4 groups connected by bridging
2322 will alter the structure and increase the configurational disorder, which are manifested
143
2323 by: (1) the occurrence of higher-coordination Al species, i.e., AlO5 and AlO6, perhaps
2324 at the expense of AlO4 by the virtual reaction, REO7 + AlO4 → REO6 + AlO5
2325 [352,356]; (2) anomalous features of free O ions and Al-O (NBO) over wider
2326 compositional ranges [344,345,356]; and (3) violations of Loewenstein’s rule by the
2328 disorder will be concurrently increased with the filed strength of RE3+ [349].
2329 Generally, RE3+ ions have been considered to play dual roles in, not only modifying
2330 the network by generating NBO, but also balancing the negatively charged AlO4 unit
2331 [348,349,352,356,360]. For example, Charpentier [349] reported that RE3+ in the
2332 alkaline earth-aluminosilicate glass exhibits dual functionality, i.e., decreasing the
2333 polymerization like a modifier at high temperature but strengthening the glass
2334 network at lower temperature. Therefore, when considering the REY diffusion
2335 mechanisms during coal combustion, the combustion temperature and coal
2336 mineralogy including the mineral types and mineral-mineral associations should be
2337 considered.
2338
144
2339
2340 Figure 37. A structural yttrium (Y)-aluminosilicate glass model, showing how the
2341 [YOx] polyhedral interconnect with their neighboring units through O. Unit 1 is an
2342 [YO6] octahedron sharing corners with three [SiO4] tetrahedral, and one corner each
2343 with [AlO4], [AlO5], [YO5] and [YO6] (unit 2) polyhedra, as well as edges with
2344 [AlO5], [YO5] (unit 3), and [YO7] (unit 4) groups. Totally, [YO6] shares seven corners
2345 and three edges with other cation neighbors through O. After Stevensson et al. [348].
2347
2348 To summarize, during coal combustion, the enrichment of REY in coal ash is
2349 mainly related to the REY incorporation into silicate melts and, thus, the fly ash
2350 glasses are the main hosts for REY. As shown in Figure 38, two retention
2351 mechanisms are proposed in this review. The capture of REY-bearing trace phases
2352 into glass is manifested by the direct observation of micro- and nano-sized
2355 enriched in REY, REY-bearing trace phases are less common in coal ash than in the
2356 parent coal. This might be explained by the size reduction of the REY trace phases
2357 into nano-sized particles due to thermal shock [144,192]. The uniform
2358 chondrite-normalized REE distribution patterns for various fly ash constituents versus
2359 bulk ash [146] and the consistent bulk Ce [232] or Y [145,233] XANES of fly ash
2360 samples resembling Ce-, Y-doped aluminosilicates argue against REY occurrences as
2361 randomly captured and distributed sub-micron domains. Diffusion of REY from trace
2362 phases to the aluminosilicate glass might be another REY capture mechanism. Similar
2364 melt system, but the diffusion mechanism for enriching REY in coal ash seems to be
2365 elusive. In a coal-fired power plant, thermal maxima last on the order of 1-2s, whereas
2366 times in diffusion of RE2O3 into silicate glass is generally longer (15 min or more).
2367 Thus, diffusion of trace REE phases might be difficult in coal combustion systems.
2368 Overall, current research data is still insufficient for a full understanding of REY
2370 whether the physical encapsulation or diffusion mechanism dominate the REY
2371 incorporation process during coal combustion. This is because the location and
2372 structure of REY in glasses greatly influence the extraction efficiency of REY from
2373 coal ash, which is reflected in the chemical durability of the aluminosilicate glass.
2374 Rare earth-bearing glasses, if the diffusion mechanism dominates, the extraction of fly
146
2375 ash glass might be more difficult because rare earth cations in the glass network can
2376 increase the water, acid, and alkaline resistance of glass [361,362].
2377
2378
2379 Figure 38. An overview of REY retention mechanisms by ash glass during coal
2380 combustion.
2381
2384 illustrated in Figure 39. The mass balance of REY is an average value based on the
2385 field sampling data from Li et al. [28] as an example explaining the REY fate in
2386 power plant. As shown in Figure 39, due to the high boiling temperature, REY in coal
2387 is hardly volatilized and therefore the stack emission of REY from coal-fired power
2388 plants is negligible. In contrast, most of REY will partition into coal ash. Generally,
2389 unlike volatile trace elements (such as Hg, As, and Se), REY entering the coal-fired
147
2390 boiler seems not be systematically fractionated between coal, fly ash, and bottom ash.
2391 Nonetheless, the relative higher mass percentages of REY in fly ash than bottom ash
2392 can be observed, probably resulting from the (1) the ratio of fly ash to bottom ash
2393 produced in coal combustion process is usually about 4:1; and (2) higher REY
2394 concentrations in fly ash than in bottom ash. Likewise, little partitioning between the
2395 ash-collection rows is observed. However, variation in the light versus heavy REE has
2396 been noted between ESP rows and among sized fractions of fly ashes. Currently, it is
2397 still not clear what is behind the phenomenon, and two reasons may account for it: (1)
2398 HREE have preferences for organic matter in coal, leading to HREE enrichment in
2399 finer fly ash particles via a more intense vaporization-condensation process during
2400 coal combustion; (2) finer fly ash particles from back-rows of ESP system may
2401 contain more glass components than that of the coarse particles from the first ESP
2402 rows.
2403 Detailed partitioning mechanisms of REY from coal to the solid ash involve
2404 thermal decomposition of various REE species in coal, mineral fragmentation, and
2405 incorporation of REY species into silicate melts at furnace temperature (Figure 39).
2406 Most of REY in coal occurs as thermally stable minerals such as REY phosphates and
2407 silicates, indicating that some REY trace phases in coal may survive and remain intact
2408 in the combustion process. However, one cannot readily reach the conclusions that
2409 REY will not be subject to vaporize-condensation process and other thermal reactions
2410 during coal combustion, because 1) some of REY in coal occur as thermal unstable
2411 compounds, such REY-bearing carbonates and organic-associated REY (Table 3); 2)
148
2412 different REY have their special thermal properties and reactivities, as can be
2413 reflected in their wide boiling-point range (1193-3454 °C; Figure 27); and 3) even
2414 for the thermal stable REY-bearing minerals, these minerals, along with other “active”
2415 minerals included within one coal particle can coalesce and react at a
2416 high-temperature condition (Figure 38). It is commonly observed that REY occur in
2418 The partitioning of REY species into aluminosilicate glass is controlled by (1)
2419 variation in coal origins / sources, both resulting in different coal mineralogical
2420 characteristics and different feed coal chemistry affecting the glass formation; (2)
2421 variations during ash formation and collection at coal-fired power plant, such as the
2422 combustion conditions of the boiler, load, ash collection device configurations, etc.
2423 After coal combustion, the interactions between REY in fly ash and flue gas
2424 compositions may further influence the final speciation of REY in coal ash.
2425
149
2426
2427 Figure 39. An overview of REY partitioning behavior during coal combustion in power plants. The mass fractions of REY (%) in coal,
2428 adsorbents (limestone), bottom ash, fly ash, FGD gypsum, and in stack gas are compiled from Li et al. [28].
2429
150
2430 7. Methods for REY recovery from coal ash
2432 Many laboratory experimental studies have been conducted in recent years to
2433 recover REY from coal combustion ash, and the investigated methods can be
2436 roasting with the addition of appropriate additives has also been employed in
2438 REE from coal combustion ash [107,165,366]. As reported in the literature, the
2439 highest content of REY in coal combustion ash, especially coal fly ash, is usually
2441 [23,33,108,175]. Therefore, preconcentrates containing more REY relative to feed ash
2442 materials can be obtained using physical beneficiation methods, such as sieving,
2446 shown in Table 20, preconcentrates of higher REY content have been generated from
2447 several coal fly ashes through physical beneficiation; however, the enrichment ratios
2448 of REY content in the preconcentrates to that in the feeds are exceedingly low. This
2449 fact suggested the low efficiency of using physical beneficiation to preconcentrate
2450 REY from coal combustion ash. In order to achieve a higher enrichment ratio and
2451 produce a product of higher grade, different physical beneficiation methods can be
151
2452 collectively applied. For example, Blissett et al. [23] obtained a product containing
2453 637 ppm of REY from a fly ash with 505 ppm of REY, using flotation, magnetic
2454 separation, and classifying cyclone to remove unburned carbon, magnetic particles,
2455 and coarse particles, respectively. Pan et al. [108] used a process consisting of size
2457 Non-magnetic material containing 1025 ppm of REY was obtained from a fly ash
2458 with 782 ppm of REY. Using preconcentrated coal combustion ash as a higher-grade
2459 feedstock reduces the cost for REY recovery. Besides, physical beneficiation can (1)
2460 produce a more uniform feed to the chemical processing, (2) eliminate oversize
2461 material that would be inefficient to process, (3) eliminate carbons that can adsorb
2462 chemicals, and (4) eliminate magnetics which usually have lower REY.
2463
2464 Table 20. A summary of the physical beneficiation of REE from coal fly ash
2465 (Conc., ER, and Re represent the content, enrichment ratio, and recovery of REE in
Conc. Re
Sample Location Recovery Method ER Reference
-1
(µg g ) (%)
152
Density fractionation 522 1.02 95
2467 Note: Con, ER, and Re represent content, enrichment ratio, and recovery, respectively.
2468
2470 While REY can be enriched from coal combustion ash using physical
2473 further processed for purification and upgrading. However, due to the inclusion of
2474 REY in the glassy matrix of coal combustion ash, the leaching recovery of REY is
2475 normally low and harsh reaction conditions are required [107,122,365,367]. As
2476 reported in a study performed on a fly ash sample collected from a Chinese power
2477 plant, less than 20% of total rare earth elements were leached using 12M HCl or 16M
2478 HNO3 [367]. The low leaching recovery of REE agrees with findings from sequential
2480 majority of REE in coal combustion ash is associated with aluminum-silicate phases
2481 which can only be dissolved by digestion. However, there are some exceptions.
2482 Nearly 100% of rare earth recovery has been achieved for high calcium-containing fly
2483 ashes such as samples derived from Power River Basin coals in the U.S. [364]. Coal
2484 combustion ashes generated from fluidized bed combustors showed relatively high
2485 leachabilities, likely due to the lower combustion temperatures than pulverized or
2487 Given the low leachability of REY in most fly ashes, pretreatment by roasting
2488 with additives (e.g., NaOH, Na2CO3, and CaO) or reacting with strong alkaline
2489 solutions have been applied to dissolve REY from ash into solution
2491 combustion ash is destroyed, and difficult-to-leach rare earth minerals such as
2492 monazite are decomposed, collectively contributing towards high REY recoveries. For
2493 example, Taggart et al. [165] compared different roasting additives and found that
154
2494 NaOH and Na2O2 performed better than other chemicals, and >90% of total REY can
2495 be recovered followed by leaching under mild conditions such as 1-2M HNO3. Strong
2496 alkaline solutions, such as 6.25 M NaOH [364], 3 M NaOH [369], and 40% NaOH
2497 [27], are able to decompose aluminum-silicate glassy matrix into soluble species, such
2499 encapsulated in the matrix can be released and mostly converted into rare earth
2500 hydroxides under such strong alkaline conditions [372], which can be easily leached
2501 under weakly acidic conditions. Based on the above discussions, the most effective
2502 way to recover REY from coal combustion ash is combining physical and chemical
2504 particles of different physical natures, a high-grade feed material can be obtained from
2505 coal combustion ash for downstream pretreatment and acid leaching processes. Using
2506 this concept, Pan et al. [108] developed a process, consisting of size classification,
2507 magnetic separation, roasting, and acid leaching units, which enables 80% of REY in
2509 Nearly all existing studies reported in the literature failed to incorporate
2510 economic analysis. This analysis is essential for the commercial deployment of
2512 results. As shown in Table 21, nearly all the hydrometallurgical and pyrometallurgical
2513 methods reported in the literature consume an exceedingly high dosage of chemicals,
2514 suggesting that operating costs for the recovery of REY from coal combustion ash
2515 will be high, leading to low economic viability. The situation is worsened by the fact
155
2516 that as an alternate resource, coal combustion ash has a much lower REY content
2517 relative to conventional rare earth ore deposits. As presented in a report by [373], the
2518 per tonne cost to process fly ash in a commercial plant using alkaline followed by acid
2519 leaching is approximately $140. This cost is too high to make the recovery
2520 economically viable if only REE is produced as the saleable product. In order to
2521 improve the economic viability for REE recovery from coal combustion ash, it needs
2522 to be combined with other beneficial uses, such as aluminum recovery and zeolite
2523 production [374,375]. A technical roadmap for recovering REY from coal combustion
2524 ash is presented in Figure 40. Different options are available, such as
2527 For a specific ash material, a comprehensive experimental program is required to find
2529
2530 Table 21. Studies reported in the literature with higher recoveries of REY from
Fly ash USA Reacting with 6.25 mol/L REY recoveries of up [364]
Fly ash USA Reacting with 5 mol/L NaOH REY was enriched [176]
Fly ash USA Roasting with NaOH (1:1 by REY recoveries [233]
156
acid leaching with 1-2 mol/L obtained for all ash
HNO3 samples
Fly ash China Roasting with Na2CO3 (1:1 by A REY recovery of [107]
HCl
Fly ash China Reacting with a 40% NaOH A REY recovery of [27]
HCl
Fly ash USA Roasting with Na2CO3 (1:1 by >90% of REY was [366]
Fly ash China Reacting with 3 mol/L NaOH A REY recovery of [369]
2532
157
2533
2534 Figure 40. Technical roadmap for REY recovery from coal combustion ash
2535 formulated based on findings from existing studies reported in the literature.
2536
2537 8. Conclusions
2538 Coal ash is one of the most promising sources for rare earth elements and yttrium
2539 (REY). The present work aims for (1) making a comprehensive summary of REY
2540 contents, distribution, speciation, and analytical methods for REY in coal ash; (2) a
2542 transformation and retention mechanisms during coal combustion; and (3) the recovery
2543 methods developed in recent years. The distribution of REY among various streams
2544 across the whole power plants and the retention mechanisms of REY by fly ash glasses
2546 The most fundamental control on REY in coal ash is their amount in the parent
158
2547 coal. REY in coal is most commonly in phosphate minerals but can occur in a number
2548 of other minerals (carbonates, silicates, etc.) as “included” minerals and in organic
2549 association in low-rank coals. The concentration of REY greatly varies in different coal
2550 deposits or even coal seams, and the combustion of “metalliferous coal” can produce
2551 REY-rich ash meeting the cut-off grade for industrial extraction. A detailed knowledge
2552 of REY in feed coals is essential for providing both a background and basis for
2554 Methods to characterize REY in coal ash can inform REY extraction strategies.
2555 A summary and comparison on the advantages and limitations of various methods for
2556 determining REY contents and speciation is made in this study. Methods that are used
2557 for total REY content determinations mainly include ICP-MS, followed by ICP-OES,
2558 INAA, and XRF. ICP-MS is recommended for determining REY in coal ash because
2559 of its high sensitivity and multi-elemental capability. INAA could be a reference
2560 method for estimating the precision and accuracy in determination of REY by other
2561 techniques. XRF, as a rapid and nondestructive method for analysis of solid sample, is
2562 suitable for field survey screening coal ash for laboratory examination and REY
2563 recovery. Sequential leaching can quantify REY associations but often have difficulties
2565 abundant REY such as Ce and Y can be completed using synchrotron-based XANES on
2566 either the bulk- or micro-scale. However, the similar spectral features of reference
2567 materials restrict the results to qualitive descriptions. TEM is useful in analyzing
2568 nanometer-scale REY-bearing domains, which may differ considerably from macro-
159
2569 and micro-scale REY hosts.
2570 The contents and reserve of REY in coal ash are the primary factor
2571 determining the extraction potentials of REY from fly ash. This study updates the
2572 reported value from Ketris and Yudovich [82], which was obtained based on the REY
2573 contents in coal. Rather, current work compiled data of 581 coal ashes produced at
2574 coal-fired power plants from 15 countries around the world. The estimated average
2575 REY contents in world coal-derived fly ash are 435.4 µg g-1. The concentration of REY
2576 in coal ash greatly varies, which heavily depends on the geological origin of feed coal.
2577 REY contents in Chinese coal ash (473 µg g-1) and U.S. coal ash (459.61 µg g-1) are
2578 higher than those in European (278.65 µg g-1) and other countries (298 µg g-1).
2579 Coal-derived fly ashes from China and U.S. are two typical examples showing the
2580 variations of REY with feed coal origins. In comparison to coal ash from other regions,
2581 the central Appalachian basin coal-derived ashes and southwestern China coal ashes
2582 are significantly enriched REY, providing three times the critical REY of total REY
2584 The speciation of REY in coal ash is another key factor affecting the extraction
2585 efficiencies of REY from coal ash. This study classifies the speciation of REY in coal
2586 ash as amorphous glassy associations, discrete REY minerals or compounds, and as
2587 REY bound with unburned carbon. Rare earth elements are mostly found to be
2588 associated with aluminosilicate glass in coal ash. Two possible forms account for the
2589 Si-Al glassy associations, i.e., individual REY-bearing phases that are closely bound
2590 with aluminosilicate glasses and REY dispersed throughout the fly ash glass. The
160
2591 former association has been extensively demonstrated via electron microscopy
2593 means of ion microprobe indicate that REY in fly ash samples is dispersed into Si-Al
2594 glasses formed during melting at boiler temperatures. Discrete REY minerals are
2595 usually more difficult to be detected in coal ash than that in coal, with particle size
2596 ranging from several microns to ~nm, or even to sub-nanometers (as shown by TEM).
2597 The association of REY with unburned carbon is difficult to be distinguished. Only
2598 nanosized particles containing REY are found in amorphous and graphitic carbons
2600 Rare earth elements and yttrium are not volatile elements; and their mass
2601 distributions among different emission streams in power plants show an enrichment in
2602 the combustion ash, especially in fly ash. There is no significant REY fractionation
2603 among different ESP fly ashes or in the sized ash based on their normalized distribution
2604 pattern relative to the upper continental crust (UCC). However, a significant variation
2605 in the light REE versus heavy REE is noted between ESP rows and among sized
2606 fractions of fly ashes. Variations in the amount and size of REY minerals between and
2609 The speciation of REY in coal can be greatly altered during and after coal
2610 combustion. The thermally stable REY-bearing minerals, such as phosphates, silicates,
2611 etc. in coal may not melt at boiler but, instead, shatter into very fine grains. Thermal
161
2613 water-bearing REY phosphates and sulfates, and other minerals have been observed in
2614 both pure mineral combustion experiments and direct XANES determinations. Most of
2615 REY is retained in aluminosilicate glass with very few REY phases emitted as gaseous
2616 forms. The heat-induced fragmented REY minerals, neo-formed minerals, or the
2617 original REY minerals in coal are partitioned into the Al-Si glass by two mechanisms:
2618 the incorporation of the individual REY phases into the glass as inclusions and the
2619 diffusion of REE phases throughout Si-Al glass structures in the melting process. The
2620 retention of REY by aluminosilicate glass is controlled by the feed-coal mineral types,
2621 mineral-mineral associations, boiler conditions, etc. After coal combustion at boiler
2622 temperatures, the speciation of REY in may be further influenced and modified by the
2624 REY recovery from coal combustion ash normally requires harsh conditions
2625 because of the encapsulation of REY-rich particles in the glassy matrix. Various
2626 methods have been tested in existing studies, such as physical beneficiation, roasting,
2627 alkaline leaching, and acid leaching. Based on the review, using physical beneficiation
2628 first to generate concentrates with higher REY content followed by hydrometallurgical
2631 A number of works have been devoted to the REY contents in coal, but the
2632 contents in coal ash, especially the REY contents in the ponded ash are not known.
2633 Portable XRF has been developed for screening coal ashes for REY recovery in field
2634 survey, but its precision and accuracy should be further improved.
162
2635 While a number of techniques have been used to determine the REY
2636 associations in coal or coal ash, methods that can be used for quantifying various REY
2637 associations in coal or coal ash should be developed. The quantification of REY
2638 minerals in coal by CCSEM is a good start, but the size and the trace amounts of REY
2639 phases (at ~ µg g-1 or sub-µg g-1 level) in heterogenous coal ash make the
2641 The current TEM studies observed the nanosized REY inclusions occurring
2642 in the bituminous coal-derived fly ash. More research and studies are needed for
2643 confirming those associations by extending the work to higher and lower coal ranks.
2644 Current studies have investigated the high-temperature reactions of pure REY
2645 species are limited to below 1000 ℃ and in an air atmosphere, future work on
2646 behavior of the main REY species in coal at a wider temperature range, a more
2647 oxidizing and reducing atmosphere, and in the presence of acid gas components
2649 One of the main reasons for a lower extraction efficiency of REY from coal
2650 ash in particular Class F fly ash is that most of REY partitioned into aluminosilicate
2651 glasses in the combustion process. The ash glass reactivities including their
2652 dissolution rates and chemical durability are determined by the fly ash glass structures
2653 and compositions. Initial fundamental work on the diffusion of REY into glasses in
2654 coal ash should determine what types of glasses host REY in coal ash and the
163
2657 Recovery of REY from coal combustion ash is viable from a technical point
2658 of view per existing studies; however, the economic viability of REY recovery from
2659 coal combustion ash has not been sufficiently assessed. More efforts are required to
2660 evaluate capital and operating expenses to generate a certain quantity of REY.
2661 Moreover, REY recovery needs to be combined with other beneficial uses of coal
2662 combustion ash, such as aluminum recovery, zeolite preparation, and supplementary
164
2664 Acknowledgements
2665 This work was supported by the National Natural Science Foundation of China
2666 (52006082) and Chinese Postdoctoral Science Foundation (2019M662586). This study
2667 was completed as part of U.S. Department of Energy contracts DE-FE0027167 and
2669 University of North Dakota Energy & Environmental Research Center with a
2670 subcontract to the University of Kentucky; and U.S. National Science Foundation
2671 grants CBET-1510965 and CBET-1510861 to Duke University and the University of
2672 Kentucky, respectively. This work used shared facilities at the Virginia Tech National
2675 supported by NSF (ECCS 1542100). Additional microbeam analyses were conducted
2677
2678
2679
2680
2681
2682
2683
2684
165
2685 References
2686 [1] Jensch E. On the metal content of Upper Silesian coals. Chem Ind Berl 1887;10.
2687 [2] Goldschmidt VM. Rare elements in coal ashes. Ind Eng Chem 1935;27:1100–2.
2688 [3] Swaine DJ. Trace elements in coal. Butterworth-Heinemann Ltd, Oxford, UK.;
2689 1991.
2691 [5] Thompson AP, Musgrave JR. Germanium, produced as a byproduct, has become of
2693 [6] Seredin V V., Finkelman RB. Metalliferous coals: A review of the main genetic and
2695 https://doi.org/10.1016/j.coal.2008.07.016.
2696 [7] Seredin V V., Dai S, Sun Y, Chekryzhov IY. Coal deposits as potential alternative
2697 sources for lanthanides and yttrium. Int J Coal Geol 2012;94:67–93.
2698 https://doi.org/10.1016/j.coal.2011.11.001.
2699 [8] Dai S, Yan X, Ward CR, Hower JC, Zhao L, Wang X, et al. Valuable elements in
2701 https://doi.org/10.1080/00206814.2016.1197802.
2702 [9] Seredin V V., Dai S, Sun Y, Chekryzhov IY. Coal deposits as promising sources of
2703 rare metals for alternative power and energy-efficient technologies. Appl Geochemistry
2705 [10] Massari S, Ruberti M. Rare earth elements as critical raw materials: Focus on
2707 [11] Chegwidden J, Kingsnorth DJ. Rare Earths—An Evaluation of Current and Furture
2708 Supply. Int Assoc Genocide Sch New Salem, MA, Accessed Apr 2011;3:2018.
2709 [12] Hower JC, Groppo JG, Joshi P, Preda D V., Gamliel DP, Mohler DT, et al.
2710 Distribution of lanthanides, yttrium, and scandium in the pilot-scale beneficiation of fly
2712 https://doi.org/10.3390/min10020105.
166
2713 [13] Zhang W, Noble A, Yang X, Honaker R. Lithium leaching recovery and
2714 mechanisms from density fractions of an Illinois Basin bituminous coal. Fuel
2716 [14] Hower JC, Qian D, Briot NJ, Hood MM, Eble CF. Mineralogy of a rare earth
2717 element-rich Manchester coal lithotype, Clay County, Kentucky. Int J Coal Geol
2719 [15] Honaker RQ, Zhang W, Werner J. Acid Leaching of Rare Earth Elements from Coal
2720 and Coal Ash: Implications for Using Fluidized Bed Combustion to Assist in the Recovery
2722 https://doi.org/10.1021/acs.energyfuels.9b00295.
2723 [16] Taggart RK, Hower JC, Dwyer GS, Hsu-Kim H. Trends in the Rare Earth Element
2724 Content of U.S.-Based Coal Combustion Fly Ashes. Environ Sci Technol 2016;50:5919–26.
2725 https://doi.org/10.1021/acs.est.6b00085.
2726 [17] Hower JC, Granite EJ, Mayfield DB, Lewis AS, Finkelman RB. Notes on
2727 contributions to the science of rare earth element enrichment in coal and coal combustion
2730 potential of polish fly ashes as a source of rare earth elements. Ore Geol Rev
2731 2020;124:103638.
2732 [19] Valentim B, Abagiu AT, Anghelescu L, Flores D, French D, Gonçalves P, et al.
2733 Assessment of bottom ash landfilled at Ceplea Valley (Romania) as a source of rare earth
2736 coal-combustion ashes prior to and after their leaching in HCl. Fuel Process Technol
2738 [21] Lanzerstorfer C. Fly ash from coal combustion: Dependence of the concentration of
2740 https://doi.org/10.1016/j.fuel.2018.04.136.
2741 [22] Folgueras MB, Alonso M, Fernández FJ. Coal and sewage sludge ashes as sources of
2744 the United Kingdom and Poland to evaluate rare earth element content. Fuel 2014;119:236–
2745 9. https://doi.org/10.1016/j.fuel.2013.11.053.
2746 [24] Dai S, Zhao L, Hower JC, Johnston MN, Song W, Wang P, et al. Petrology,
2747 mineralogy, and chemistry of size-fractioned fly ash from the Jungar power plant, Inner
2748 Mongolia, China, with emphasis on the distribution of rare earth elements. Energy and Fuels
2750 [25] Liu H. Compostion of the coal combustion and utilization of the fly ash generated
2751 from two major coal-fired power plants in Chongqing city, Southwest China. Ph.D Thesis.
2753 [26] Pan J, Zhou C, Liu C, Tang M, Cao S, Hu T, et al. Modes of Occurrence of Rare
2754 Earth Elements in Coal Fly Ash: A Case Study. Energy and Fuels 2018;32:9738–43.
2755 https://doi.org/10.1021/acs.energyfuels.8b02052.
2756 [27] Wang Z, Dai S, Zou J, French D, Graham IT. Rare earth elements and yttrium in coal
2757 ash from the Luzhou power plant in Sichuan, Southwest China: Concentration,
2759 https://doi.org/10.1016/j.coal.2019.01.001.
2760 [28] Li Z, Li X, Zhang L, Li S, Chen J, Feng X, et al. Partitioning of rare earth elements
2761 and yttrium (REY) in five coal-fired power plants in Guizhou, Southwest China. J Rare
2763 [29] Seredin V V. Rare earth element-bearing coals from the Russian Far East deposits.
2765 [30] Kumari A, Parween R, Chakravarty S, Parmar K, Pathak DD, Lee J chun, et al.
2766 Novel approach to recover rare earth metals (REMs) from Indian coal bottom ash.
2768 [31] Mondal S, Ghar A, Satpati AK, Sinharoy P, Singh DK, Sharma JN, et al. Recovery
2769 of rare earth elements from coal fly ash using TEHDGA impregnated resin.
168
2771 [32] Wagner NJ, Matiane A. Rare earth elements in select Main Karoo Basin (South
2772 Africa) coal and coal ash samples. Int J Coal Geol 2018;196:82–92.
2773 https://doi.org/10.1016/j.coal.2018.06.020.
2774 [33] Rosita W, Bendiyasa IM, Perdana I, Anggara F. Sequential particle-size and
2775 magnetic separation for enrichment of rare-earth elements and yttrium in Indonesia coal fly
2777 [34] Dai S, Graham IT, Ward CR. A review of anomalous rare earth elements and yttrium
2779 [35] Hower JC, Eble CF, Dai S, Belkin HE. Distribution of rare earth elements in eastern
2780 Kentucky coals: Indicators of multiple modes of enrichment? Int J Coal Geol 2016;160–
2782 [36] Hower JC, Ruppert LF, Eble CF. Lanthanide, yttrium, and zirconium anomalies in
2783 the Fire Clay coal bed, Eastern Kentucky. Int J Coal Geol 1999;39:141–53.
2784 https://doi.org/10.1016/S0166-5162(98)00043-3.
2785 [37] Dai S, Xie P, Jia S, Ward CR, Hower JC, Yan X, et al. Enrichment of U-Re-V-Cr-Se
2786 and rare earth elements in the Late Permian coals of the Moxinpo Coalfield, Chongqing,
2787 China: Genetic implications from geochemical and mineralogical data. Ore Geol Rev
2789 [38] Dai S, Liu J, Ward CR, Hower JC, French D, Jia S, et al. Mineralogical and
2790 geochemical compositions of Late Permian coals and host rocks from the Guxu Coalfield,
2791 Sichuan Province, China, with emphasis on enrichment of rare metals. Int J Coal Geol
2793 [39] Dai S, Xie P, Ward CR, Yan X, Guo W, French D, et al. Anomalies of rare metals in
2794 Lopingian super-high-organic-sulfur coals from the Yishan Coalfield, Guangxi, China. Ore
2797 and Promising Recovery Methods of Rare Earth Elements from A Review of the Occurrence
2798 and Promising from Coal and Coal By-Products. Int J Coal Prep Util ISSN 2015;35:295–
169
2800 [41] Borzone G, Raggio R, Ferro R. Thermochemistry and reactivity of rare earth metals.
2802 [42] Hower JC, Groppo JG, Henke KR, Hood MM, Eble CF, Honaker RQ, et al. Notes on
2803 the potential for the concentration of rare earth elements and yttrium in coal combustion fly
2805 [43] Bao Z, Zhao Z. Geochemistry of mineralization with exchangeable REY in the
2806 weathering crusts of granitic rocks in South China. Ore Geol Rev 2008;33:519–35.
2807 [44] McLellan BC, Corder GD, Ali SH. Sustainability of rare earths—An overview of the
2809 [45] Zhao Z, Cui L, Guo Y, Li H, Cheng F. Recovery of gallium from sulfuric acid leach
2810 liquor of coal fly ash by stepwise separation using P507 and Cyanex 272. Chem Eng J
2812 [46] Zhang W, Yang X, Honaker RQ. Association characteristic study and preliminary
2813 recovery investigation of rare earth elements from Fire Clay seam coal middlings. Fuel
2815 [47] Damhus T, Hartshorn RM, Hutton AT. Nomenclature of inorganic chemistry:
2817 [48] Li C, Lin J. Rare earth fluoride nano-/microcrystals: synthesis, surface modification
2819 [49] Tan TTY. Rare earth nanotechnology. 1st Editio. Jenny Stanford Publishing; 2012.
2820 https://doi.org/10.1201/b12310.
2821 [50] Lian H, Hou Z, Shang M, Geng D, Zhang Y, Lin J. Rare earth ions doped phosphors
2823 https://doi.org/10.1016/j.energy.2013.05.019.
2824 [51] Pan H, Ren Y, Fu H, Zhao H, Wang L, Meng X, et al. Recent developments in
2825 rare-earth free wrought magnesium alloys having high strength: A review. J Alloys Compd
2827 [52] Akah A. Application of rare earths in fluid catalytic cracking: A review. J Rare
170
2829 [53] Cheisson T, Schelter EJ. Rare earth elements: Mendeleev’s bane, modern marvels.
2831 [54] Zhao H, Xia J, Yin D, Luo M, Yan C, Du Y. Rare earth incorporated electrode
2832 materials for advanced energy storage. Coord Chem Rev 2019;390:32–49.
2833 https://doi.org/10.1016/j.ccr.2019.03.011.
2834 [55] Gammons CH, Wood SA, Jonas JP, Madison JP. Geochemistry of the rare-earth
2835 elements and uranium in the acidic Berkeley Pit lake, Butte, Montana. Chem Geol
2837 [56] Wood SA, Williams-Jones AE. The aqueous geochemistry of the rare-earth elements
2838 and yttrium 4. Monazite solubility and REE mobility in exhalative massive
2840 https://doi.org/10.1016/0009-2541(94)90144-9.
2841 [57] Wood SA. The aqueous geochemistry of the rare-earth elements and yttrium. 1.
2842 Review of available low-temperature data for inorganic complexes and the inorganic REE
2844 https://doi.org/10.1016/0009-2541(90)90080-Q.
2845 [58] Peccerillo A, Taylor SR. Geochemistry of eocene calc-alkaline volcanic rocks from
2846 the Kastamonu area, Northern Turkey. Contrib to Mineral Petrol 1976;58:63–81.
2847 https://doi.org/10.1007/BF00384745.
2848 [59] Peng S, Kusky TM, Jiang XF, Wang L, Wang JP, Deng H. Geology, geochemistry,
2849 and geochronology of the Miaowan ophiolite, Yangtze craton: Implications for South
2850 China’s amalgamation history with the Rodinian supercontinent. Gondwana Res
2852 [60] Hidayah NN, Abidin SZ. The evolution of mineral processing in extraction of rare
2853 earth elements using liquid-liquid extraction: A review. Miner Eng 2018;121:146–57.
2854 https://doi.org/10.1016/j.mineng.2018.03.018.
2855 [61] Jordens A, Cheng YP, Waters KE. A review of the beneficiation of rare earth
2857 https://doi.org/10.1016/j.mineng.2012.10.017.
171
2858 [62] Neumann R, Medeiros EB. Comprehensive mineralogical and technological
2859 characterisation of the Araxá (SE Brazil) complex REE (Nb-P) ore, and the fate of its
2861 https://doi.org/10.1016/j.minpro.2015.08.009.
2862 [63] Borai EH, El-Ghany MSA, Ahmed IM, M.Hamed M, El-Din AMS, Aly HF.
2863 Modified acidic leaching for selective separation of thorium, phosphate and rare earth
2864 concentrates from Egyptian crude monazite. Int J Miner Process 2016;149:34–41.
2865 https://doi.org/10.1016/j.minpro.2016.02.003.
2866 [64] Schulz B, Merker G, Gutzmer J. Automated SEM mineral liberation analysis (MLA)
2867 with generically labelled EDX spectra in the mineral processing of rare earth element ores.
2869 [65] Migaszewski ZM, Gałuszka A. The characteristics, occurrence, and geochemical
2870 behavior of rare earth elements in the environment: A review. Crit Rev Environ Sci Technol
2873 review and an attempt to derive water and sediment quality criteria. Ecotoxicol Environ Saf
2875 [67] Ramos SJ, Dinali GS, Oliveira C, Martins GC, Moreira CG, Siqueira JO, et al. Rare
2876 Earth Elements in the Soil Environment. Curr Pollut Reports 2016;2:28–50.
2877 https://doi.org/10.1007/s40726-016-0026-4.
2878 [68] United States Environmental Protection Agency. Rare Earth Elements : A Review of
2881 [69] Rim KT. Effects of rare earth elements on the environment and human health: A
2883 https://doi.org/10.1007/s13530-016-0276-y.
2884 [70] Zhang FS, Yamasaki S, Kimura K. Rare earth element content in various waste ashes
2885 and the potential risk to Japanese soils. Environ Int 2001;27:393–8.
2886 https://doi.org/10.1016/S0160-4120(01)00097-6.
172
2887 [71] Wei B, Li Y, Li H, Yu J, Ye B, Liang T. Rare earth elements in human hair from a
2889 https://doi.org/10.1016/j.ecoenv.2013.05.031.
2890 [72] Eskenazy GM. Aspects of the geochemistry of rare earth elements in coal: An
2892 https://doi.org/10.1016/S0166-5162(98)00027-5.
2893 [73] Schofield A, Haskin L. Rare-earth distribution patterns in eight terrestrial materials.
2895 https://doi.org/10.1016/0016-7037(64)90117-6.
2896 [74] Seredin V V., Chekryzhov IY. Ore potentiality of the Vanchin Graben, Primorye,
2898 [75] Hatch GP. Dynamics in the global market for rare earths. Elements 2012;16:295–6.
2899 https://doi.org/10.2113/gselements.8.5.341.
2900 [76] Paulick H, Machacek E. The global rare earth element exploration boom: An
2901 analysis of resources outside of China and discussion of development perspectives. Resour
2903 [77] Ding K. The rare earth magnet industry and rare earth price in China. EPJ Web Conf.,
2905 [78] Baldi L, Peri M, Vandone D. Clean energy industries and rare earth materials:
2907 https://doi.org/10.1016/j.enpol.2013.10.067.
2908 [79] Lucas J, Lucas P, Le Mercier T, Rollat A, Davenport W. Rare Earth Production, Use
2910 [80] Oddo G. Die molekularstruktur der Radioaktiven atome. Zeitschrift Für Anorg
2912 [81] Harkins WD. The Evolution of the Elements and the Stability of Complex Atoms. J
2914 [82] Ketris MP, Yudovich YE. Estimations of Clarkes for Carbonaceous biolithes: World
2915 averages for trace element contents in black shales and coals. Int J Coal Geol 2009;78:135–
2919 [84] Taylor SR, McLennan SM. The Continental Crust: its Composition and Evolution.
2920 An Examination of the Geochemical Record Preserved in Sedimentary Rocks. 1st ed.
2922 [85] Gromet LP, Haskin LA, Korotev RL, Dymek RF. The “North American shale
2923 composite”: Its compilation, major and trace element characteristics. Geochim Cosmochim
2925 [86] Haley BA, Klinkhammer GP, McManus J. Rare earth elements in pore waters of
2927 https://doi.org/10.1016/j.gca.2003.09.012.
2928 [87] Hanchar JM, van Westrenen W. Rare earth element behavior in zircon-melt systems.
2930 [88] David A. The Rare Earth Elements: Fundamentals and Applications. 1st ed. Wiley
2932 [89] Chakhmouradian AR, Wall F. Rare earth elements: Minerals, mines, magnets (and
2934 [90] Tyler G. Rare earth elements in soil and plant systems - A review. Plant Soil
2936 [91] Wang W, Qin Y, Sang S, Zhu Y, Wang C, Weiss DJ. Geochemistry of rare earth
2937 elements in a marine influenced coal and its organic solvent extracts from the Antaibao
2939 https://doi.org/10.1016/j.coal.2008.08.012.
2940 [92] Dai S, Zhou Y, Zhang M, Wang X, Wang J, Song X, et al. A new type of Nb (Ta)–
2941 Zr (Hf)–REE–Ga polymetallic deposit in the late Permian coal-bearing strata, eastern
2942 Yunnan, southwestern China: Possible economic significance and genetic implications. Int J
2945 mineralogy and geochemistry of the Late Permian coals in the Liulong Mine of the Liuzhi
174
2946 Coalfield, Guizhou Province, Southwest China. Int J Coal Geol 2016;154–155:1–15.
2947 https://doi.org/10.1016/j.coal.2015.12.003.
2948 [94] Huang Q, Talan D, Restrepo JH, Baena OJR, Kecojevic V, Noble A.
2949 Characterization study of rare earths, yttrium, and scandium from various Colombian coal
2951 https://doi.org/10.1016/j.coal.2019.04.008.
2952 [95] Dai S, Ren D, Chou CL, Finkelman RB, Seredin V V., Zhou Y. Geochemistry of
2953 trace elements in Chinese coals: A review of abundances, genetic types, impacts on human
2955 https://doi.org/10.1016/j.coal.2011.02.003.
2956 [96] Hu J, Zheng B, Finkelman RB, Wang B, Wang M, Li S, et al. Concentration and
2957 distribution of sixty-one elements in coals from DPR Korea. Fuel 2006;85:679–88.
2958 https://doi.org/10.1016/j.fuel.2005.08.037.
2959 [97] Karayigit AI, Gayer RA, Querol X, Onacak T. Contents of major and trace elements
2960 in feed coals from Turkish coal-fired power plants. Int J Coal Geol 2000;44:169–84.
2961 https://doi.org/10.1016/S0166-5162(00)00009-4.
2962 [98] Finkelman RB. Trace and minor elements in coal. Org. Geochem., Springer; 1993, p.
2963 593–607.
2964 [99] Arbuzov SI, Chekryzhov IY, Finkelman RB, Sun YZ, Zhao CL, Il’enok SS, et al.
2965 Comments on the geochemistry of rare-earth elements (La, Ce, Sm, Eu, Tb, Yb, Lu) with
2966 examples from coals of north Asia (Siberia, Russian far East, North China, Mongolia, and
2968 [100] Dai S, Hower JC, Finkelman RB, Graham IT, French D, Ward CR, et al. Organic
2969 associations of non-mineral elements in coal : A review. Int J Coal Geol 2020;218:103347.
2970 https://doi.org/10.1016/j.coal.2019.103347.
2971 [101] Dai S, Finkelman RB. Coal as a promising source of critical elements: Progress and
2973 https://doi.org/10.1016/j.coal.2017.06.005.
175
2974 [102] Chehreh Chelgani S, Hower JC. Relationships between noble metals as potential
2975 coal combustion products and conventional coal properties. Fuel 2018;226:345–9.
2976 https://doi.org/10.1016/j.fuel.2018.04.041.
2977 [103] Dai S, Zhang W, Ward CR, Seredin V V., Hower JC, Li X, et al. Mineralogical and
2978 geochemical anomalies of late Permian coals from the Fusui Coalfield, Guangxi Province,
2979 southern China: Influences of terrigenous materials and hydrothermal fluids. Int J Coal Geol
2981 [104] Valiev YY, Gofen GI, Pachatzanov DN. Trace elements in the Jurassic anthracites of
2983 [105] Wang X, Wang X, Pan Z, Yin X, Chai P, Pan S, et al. Abundance and distribution
2984 pattern of rare earth elements and yttrium in vitrain band of high-rank coal from the Qinshui
2986 [106] Ning SZ, Huang S, Zhu S. Mineralization zoning of coal-metal deposits in China (in
2988 [107] Tang M, Zhou C, Pan J, Zhang N, Liu C. Study on extraction of rare earth elements
2989 from coal fly ash through alkali fusion – Acid leaching. Miner Eng 2019;136:36–42.
2990 https://doi.org/10.1016/j.mineng.2019.01.027.
2991 [108] Pan J, Nie T, Vaziri Hassas B, Rezaee M, Wen Z, Zhou C. Recovery of rare earth
2992 elements from coal fly ash by integrated physical separation and acid leaching.
2994 [109] Lin R, Soong Y, Granite EJ. Evaluation of trace elements in U.S. coals using the
2995 USGS COALQUAL database version 3.0. Part I: Rare earth elements and yttrium (REY).
2997 [110] Zhao L, Dai S, Nechaev VP, Nechaeva E V, Graham IT, French D, et al. Enrichment
2998 of critical elements (Nb-Ta-Zr-Hf-REE) within coal and host rocks from the Datanhao mine,
3000 [111] Dai S, Chekryzhov IY, Seredin V V., Nechaev VP, Graham IT, Hower JC, et al.
3001 Metalliferous coal deposits in East Asia (Primorye of Russia and South China): A review of
3003 https://doi.org/10.1016/j.gr.2015.07.001.
176
3004 [112] Zhuang X, Su S, Xiao M, Li J, Alastuey A, Querol X. Mineralogy and geochemistry
3005 of the Late Permian coals in the Huayingshan coal-bearing area, Sichuan Province, China.
3008 controls on the distribution of REY-Zr (Hf)-Nb (Ta) enrichment horizons in late Permian
3009 coals from the Qiandongbei Coalfield, Guizhou Province, SW China. Int J Coal Geol
3010 2020:103604.
3011 [114] Zhao L, Dai S, Graham IT, Wang P. Clay mineralogy of coal-hosted Nb-Zr-REE-Ga
3012 mineralized beds from Late Permian Strata, Eastern Yunnan, SW China: Implications for
3014 [115] Liu J, Song H, Dai S, Nechaev VP, Graham IT, French D, et al. Mineralization of
3016 southwestern China: Geochemical evidence for terrigenous input. Ore Geol Rev
3017 2019;115:103190.
3018 [116] Duan P, Wang W, Liu X, Sang S, Ma M, Zhang W. Differentiation of rare earth
3019 elements and yttrium in different size and density fractions of the Reshuihe coal, Yunnan
3021 [117] Wang Q, Yang RD, Bao M. Rare earth elements stratigraphic significance in late
3022 Permian coal measure from Bijie City, Guizhou Province, China. J Rare Earths
3023 2008;26:760–4.
3024 [118] Li D, Tang Y, Deng T, Chen K, Liu D. Geochemistry of rare earth elements in
3025 coal—a case study from Chongqing, southwestern China. Energy Explor Exploit
3026 2008;26:355–62.
3027 [119] Dai S, Zhao L, Peng S, Chou CL, Wang X, Zhang Y, et al. Abundances and
3028 distribution of minerals and elements in high-alumina coal fly ash from the Jungar Power
3030 https://doi.org/10.1016/j.coal.2009.03.005.
3031 [120] Huang Z, Fan M, Tian H. Rare earth elements of fly ash from Wyoming’s Powder
177
3033 [121] Pan J, Zhou C, Tang M, Cao S, Liu C, Zhang N, et al. Study on the modes of
3034 occurrence of rare earth elements in coal fly ash by statistics and a sequential chemical
3036 [122] Hower JC, Groppo JG, Henke KR, Graham UM, Hood MM, Joshi P, et al. Ponded
3037 and Landfilled Fly Ash as a Source of Rare Earth Elements from a Kentucky Power Plant.
3039 [123] Ren D, Zhao F, Dai S, Zhang J, Luo K. Geochemsitry of Trace Elements in coal.
3041 [124] Lin R, Bank T, Roth E, Granite E, Soong Y. Organic and inorganic association of
3043 [125] Finkelman RB, Palmer CA, Wang P. Quantification of the modes of occurrence of
3045 [126] Finkelman RB, Dai S, French D. The importance of minerals in coal as the hosts of
3047 [127] Greta E. Sorption of trace elements on xylain: An experimental study. Int J Coal
3049 [128] Yershov V. Rare earth elements in the coals of the Kizelovskii Coal Basin.
3051 [129] Seredin V V, Shpirt M. Rare earth elements in the humic substance of metalliferous
3053 [130] Finkelman R. Modes of occurrence of trace elements in coal.U.S. Geological Survey,
3055 [131] Palmer CA, Crowley SS, Mroczkowski SJ, Finkelman RB, Bullock JH. Quantifying
3056 the modes of occurence of trace elements in coal using sequential laboratory leaching
3058 [132] Finkelman RB. The origin, occurrence, and distribution of the inorganic constituents
3059 in low-rank coals. Proc. Basic Coal Sci. Work. US Dep. Energy, Houston, TX, 1982, p. 69–
3060 90.
3061 [133] Dai S, Ren D. Occurrence and sequential chemical extraction of rare earth element in
3062 coals and seam roofs. J China Univ Min Technol 2002;31:349–53.
178
3063 [134] Lin R, Bank T, Roth E, Granite E, Soong Y. Organic and inorganic association of
3064 rare earth elements in coal. 34th Annu Int Pittsburgh Coal Conf Coal - Energy, Environ
3066 [135] Hower JC, Berti D, Hochella MF, Mardon SM. Rare earth minerals in a “no tonstein”
3067 section of the Dean (Fire Clay) coal, Knox County, Kentucky. Int J Coal Geol 2018;193:73–
3069 [136] Dai S, Luo Y, Seredin V V., Ward CR, Hower JC, Zhao L, et al. Revisiting the late
3070 Permian coal from the Huayingshan, Sichuan, southwestern China: Enrichment and
3071 occurrence modes of minerals and trace elements. Int J Coal Geol 2014;122:110–28.
3072 https://doi.org/10.1016/j.coal.2013.12.016.
3073 [137] Zhao ZG, Tang XY, Li BF. Geochemistry of rare earth elements of coal in Huaibei
3075 [138] Zheng L, Liu G, Zhang H, Gao L, Xue J, Chou CL. Study on geochemistry of rare
3076 earth elements (REEs) in Permian coal from Huaibei coalfield. Geol J China Univ
3077 2006;12:41–52.
3078 [139] Dai S, Zhang W, Seredin V V., Ward CR, Hower JC, Song W, et al. Factors
3079 controlling geochemical and mineralogical compositions of coals preserved within marine
3080 carbonate successions: A case study from the Heshan Coalfield, southern China. Int J Coal
3082 [140] Zygarlicke CJ, Folkedahl BC, Nyberg CM, Feole IK, Kurz BA, Theakar NL, et al.
3083 Rare Eare elements (REEs) in U.S. coal-based resources: sampling, characterization, and
3085 study.https://edx.netl.doe.gov/dataset/rare-earth-elements-in-u-s-coal-based-resources,
3087 [141] Wall TF. Mineral matter transformations and ash deposition in pulverised coal
3089 https://doi.org/10.1016/S0082-0784(06)80132-3.
3092 https://doi.org/10.1016/j.proci.2010.09.014.
179
3093 [143] Hower JC, Berti D, Hochella MF, Rimmer SM, Taulbee DN. Submicron-scale
3094 mineralogy of lithotypes and the implications for trace element associations: Blue Gem coal,
3096 https://doi.org/10.1016/j.coal.2018.04.006.
3097 [144] Hower JC, Qian D, Briot NJ, Santillan-Jimenez E, Hood MM, Taggart RK, et al.
3098 Nano-scale rare earth distribution in fly ash derived from the combustion of the fire clay coal,
3100 [145] Liu P, Huang R, Tang Y. Comprehensive Understandings of Rare Earth Element
3101 (REE) Speciation in Coal Fly Ashes and Implication for REE Extractability. Environ Sci
3103 [146] Kolker A, Scott C, Hower JC, Vazquez JA, Lopano CL, Dai S. Distribution of rare
3104 earth elements in coal combustion fly ash, determined by SHRIMP-RG ion microprobe. Int
3106 [147] Montross SN, Verba CA, Chan HL, Lopano C. Advanced characterization of rare
3107 earth element minerals in coal utilization byproducts using multimodal image analysis. Int J
3109 [148] Karr Jr C. Analytical methods for coal and coal products. vol. III. 1st ed. Academic
3111 [149] Vourvopoulos G. Elemental Analysis of Coal and Its By-Products. 1st ed. World
3113 [150] Huggins FE. Overview of analytical methods for inorganic constituents in coal. Int J
3115 [151] Bullock JH, Cathcart JD, Betterton WJ. Analytical methods utilized by the United
3116 States Geological Survey for the analysis of coal and coal combustion by-products. U.S.
3118 [152] American Society of Testing Materials. ASTM D6357-19, Standard Test Methods
3119 for Determination of Trace Elements in Coal , Coke , and Combustion Residues from Coal
3121 Inductively Coupled Plasma Mass Spectrometry. 100 Barr Harbor Drive, PO Box C700,
180
3122 West Conshohocken, PA 19428-2959. United States: 2020.
3123 https://doi.org/10.1520/D6357-11.2.
3124 [153] Phuoc TX, Wang P, McIntyre D. Detection of rare earth elements in Powder River
3125 Basin sub-bituminous coal ash using laser-induced breakdown spectroscopy (LIBS). Fuel
3127 [154] Riley JT, Werth JL, Lewis LM, Mertens MJ. ICP analysis of coal slurries. Elem Anal
3129 [155] McCurdy DL, Wichman MD, Fry RC. Rapid coal analysis. Part II: Slurry
3130 atomization DCP emission analysis of NBS coal. Appl Spectrosc 1985;39:984–8.
3131 [156] Ng KC, Zerezghi M, Caruso JA. Direct Powder Injection of NBS Coal Fly Ash in
3132 Inductively Coupled Plasma Atomic Emission Spectrometry with Rapid Scanning
3134 https://doi.org/10.1021/ac00267a026.
3135 [157] Querol X, Whateley MKG, Fernández-Turiel JL, Tuncali E. Geological controls on
3136 the mineralogy and geochemistry of the Beypazari lignite, central Anatolia, Turkey. Int J
3138 [158] Liu J, Dai S, He X, Hower JC, Sakulpitakphon T. Size-dependent variations in fly
3139 ash trace element chemistry: Examples from a Kentucky power plant and with emphasis on
3141 https://doi.org/10.1021/acs.energyfuels.6b02644.
3142 [159] Zhang W, Honaker R. Enhanced leachability of rare earth elements from calcined
3144 https://doi.org/10.1016/j.mineng.2019.105935.
3145 [160] Zhao L, Dai S, Finkelman RB, French D, Graham IT, Yang Y, et al. Leaching
3146 behavior of trace elements from fly ashes of five Chinese coal power plants. Int J Coal Geol
3148 [161] Ma Z, Shan X, Cheng F. Distribution Characteristics of Valuable Elements, Al, Li,
3149 and Ga, and Rare Earth Elements in Feed Coal, Fly Ash, and Bottom Ash from a 300 MW
3151 https://doi.org/10.1021/acsomega.9b00280.
181
3152 [162] Zhang K, Pi Z. MT/T 1014-2006. Determination of major and miner elements in coal
3153 ash by Inductively Coupled Plasma-Atomic emission spectrometry. China National Coal
3155 [163] Zhang W, Honaker R. Characterization and recovery of rare earth elements and other
3156 critical metals (Co, Cr, Li, Mn, Sr, and V) from the calcination products of a coal refuse
3159 characteristics of rare earth elements from middlings and coarse refuse material associated
3161 https://doi.org/10.1016/j.fuel.2019.03.063.
3162 [165] Taggart RK, Hower JC, Hsu-Kim H. Effects of roasting additives and leaching
3163 parameters on the extraction of rare earth elements from coal fly ash. Int J Coal Geol
3165 [166] Lanzerstorfer C. Pre-processing of coal combustion fly ash by classification for
3167 https://doi.org/10.1016/j.egyr.2018.10.010.
3168 [167] Hower JC, Hood MM, Taggart RK, Hsu-Kim H. Chemistry and petrology of paired
3169 feed coal and combustion ash from anthracite-burning stoker boilers. Fuel 2017;199:438–46.
3170 https://doi.org/10.1016/j.fuel.2017.03.007.
3171 [168] Karayigit AI, Ozlem Y, Iserli S, Querol X, Mastalerz M, Oska R, et al. Mineralogy
3172 and geochemistry of feed coals and combustion residues from tunçbilek and eyitömer
3173 coal-fired power plants in western Turkey. Coal Combust Gasif Prod 2019:18–31.
3174 https://doi.org/10.4177/CCGP-D-18-00011.1.
3176 of the feed coals and their combustion by-products from two coal-fired power plants in
3178 https://doi.org/10.1016/j.fuel.2011.10.025.
3179 [170] Querol X, Fernández J, Soler A. Trace elements in coal and their behaviour during
182
3181 [171] Querol X, Juan R, Lopez-soler A, Fernandez-turiel JL, Ruiz CR. Mobility of trace
3183 [172] Yan X, Dai S, Graham IT, He X, Shan K, Liu X. Determination of Eu concentrations
3184 in coal, fly ash and sedimentary rocks using a cation exchange resin and inductively coupled
3186 https://doi.org/10.1016/j.coal.2018.03.009.
3188 robust microwave-assisted decomposition method for the determination of rare earth
3190 https://doi.org/10.1039/c7ay00286f.
3191 [174] American Society of Testing Materials. D4503-08,Standard Practice for Dissolution
3192 of Solid Waste by Lithium Metaborate Fusion. 100 Barr Harbor Drive, PO Box C700, West
3194 [175] Lin R, Howard BH, Roth EA, Bank TL, Granite EJ, Soong Y. Enrichment of rare
3195 earth elements from coal and coal by-products by physical separations. Fuel 2017;200:506–
3197 [176] Lin R, Stuckman M, Howard BH, Bank TL, Roth EA, Macala MK, et al. Application
3198 of sequential extraction and hydrothermal treatment for characterization and enrichment of
3199 rare earth elements from coal fly ash. Fuel 2018;232:124–33.
3200 https://doi.org/10.1016/j.fuel.2018.05.141.
3201 [177] Zhang Y, Jiang Z, He M, Hu B, Thompson RL, Bank T, et al. Determination of Trace
3202 Rare Earth Elements in Coal Fly Ash and Atmospheric Particulates by Electrothermal
3203 Vaporization Inductively Coupled Plasma Mass Spectrometry with Slurry Sampling.
3205 [178] Wei Q, Song W. Mineralogical and Chemical Characteristics of Coal Ashes from
3206 Two High-Sulfur Coal-Fired Power Plants in Wuhai, Inner Mongolia, China. Minerals
3209 and elements enrichment of magnetospheres from coal fly ashes. Fuel 2014;135:15–26.
3210 https://doi.org/10.1016/j.fuel.2014.06.033.
183
3211 [180] Wu G, Wang T, Zhang Y, Jiawe W, Weiping P. Study on the Enrichment of Rare
3212 Earth Elements Between Coals and Their By-products at Coal-fired Power Plants. Proc
3214 [181] Meier AL, Lichte FE, Briggs PH, Bullock Jr JH. Coal ash by inductively coupled
3216 Anal Methods Man Miner Resour Surv Progr US Geol Surv 1996:109.
3217 [182] Lichte FE, Meier AL, Crock JG. Determination of the Rare-Earth Elements in
3218 Geological Materials by Inductively Coupled Plasma Mass Spectrometry. Anal Chem
3220 [183] Ardini F, Soggia F, Rugi F, Udisti R, Grotti M. Comparison of inductively coupled
3221 plasma spectrometry techniques for the direct determination of rare earth elements in digests
3223 https://doi.org/10.1016/j.aca.2010.07.036.
3224 [184] Zhang W, Noble A. Mineralogy characterization and recovery of rare earth elements
3225 from the roof and floor materials of the Guxu coalfield. Fuel 2020;270.
3226 https://doi.org/10.1016/j.fuel.2020.117533.
3227 [185] Li Z, Clemens AH, Moore TA, Gong D, Weaver SD, Eby N. Partitioning behaviour
3228 of trace elements in a stoker-fired combustion unit: An example using bituminous coals
3229 from the Greymouth coalfield (Cretaceous), New Zealand. Int J Coal Geol 2005;63:98–116.
3230 https://doi.org/10.1016/j.coal.2005.02.007.
3231 [186] Eze CP, Fatoba O, Madzivire G, Ostrovnaya TM, Petrik LF, Frontasyeva M V., et al.
3232 Elemental composition of fly ash: a comparative study using nuclear and related analytical
3234 https://doi.org/10.2478/cdem-2013-0014.
3235 [187] Djingova R, Ivanova J. Determination of rare earth elements in soils and sediments
3238 [188] Jarvis I, Jarvis KE. Rare-earth element geochemistry of standard sediments: A study
3240 https://doi.org/10.1016/0009-2541(85)90078-6.
184
3241 [189] Roelandts I, Deblond A. Rare-earth element composition of Devonian sediments
3244 https://doi.org/10.1016/0009-2541(92)90053-8.
3249 et al. Ashes from bituminous coal burning in fluidized bed boilers as a potential source of
3250 rare earth elements. Gospod Surowcami Miner / Miner Resour Manag 2018;34:21–36.
3251 https://doi.org/10.24425/118652.
3252 [192] Madison M, Ross K, Ryan C, Kevin R, John G, Jason M, et al. Rare Earth Element
3253 Distribution in Fly Ash Derived from the Fire Clay Coal , Kentucky. Coal Combust Gasif
3255 [193] Vassilev S V., Vassileva CG. Contents and associations of rare earth elements and
3257 https://doi.org/10.1016/j.fuel.2019.116525.
3258 [194] Shao L, Chang L, Finkelman RB, Wang W, Liu J, Li J, et al. Distribution of rare
3259 earth elements in PM10 emitted from burning coals and soil-mixed coal briquettes. J
3261 [195] Middleton A, Park DM, Jiao Y, Hsu-kim H. Major element composition controls
3262 rare earth element solubility during leaching of coal fly ash and coal by-products. Int J Coal
3264 [196] Tang M, Zhou C, Zhang N, Pan J, Cao S, Hu T, et al. Extraction of rare earth
3265 elements from coal fly ash by alkali fusion–acid leaching: Mechanism analysis. Int J Coal
3267 [197] Ganjali MR, Gupta VK, Faridbod F, Norouzi P. Overview of Lanthanides Series
3269 https://doi.org/10.1016/b978-0-12-804704-0.00004-9.
185
3270 [198] Zawisza B, Pytlakowska K, Feist B, Polowniak M, Kita A, Sitko R. Determination of
3273 [199] Sandoval Rojano WJ, dos Anjos T, Duyck CB, Saint’Pierre TD. Determination of
3274 rare earth elements in environmental samples with high concentrations of barium by
3276 https://doi.org/10.1016/j.microc.2019.104026.
3277 [200] Thompson RL, Bank T, Roth E, Granite E. Resolution of rare earth element
3278 interferences in fossil energy by-product samples using sector-field ICP-MS. Fuel
3280 [201] Jarvis KE, Gray AL, McCurdy E. Avoidance of spectral interference on europium in
3281 inductively coupled plasma mass spectrometry by sensitive measurement of the doubly
3283 [202] Raut NM, Huang LS, Lin KC, Aggarwal SK. Uncertainty propagation through
3284 correction methodology for the determination of rare earth elements by quadrupole based
3285 inductively coupled plasma mass spectrometry. Anal Chim Acta 2005;530:91–103.
3286 https://doi.org/10.1016/j.aca.2004.08.067.
3287 [203] Vaughan MA, Horlick G. Correction procedures for rare earth element analyses in
3289 [204] Riondato J, Vanhaecke F, Moens L, Dams R. Determination of rare earth elements in
3292 [205] Vaughan MA, Horlick G. Effect of sampler and skimmer orifice size on analyte and
3293 analyte oxide signals in inductively coupled plasma-mass spectrometry. Spectrochim Acta
3295 [206] Louie H, Soo SY-P. Use of nitrogen and hydrogen in inductively coupled plasma
3297 [207] Tao H, Miyazaki A. Decrease of solvent water loading in inductively coupled
3298 plasma mass spectrometry by using a membrane separator. J Anal At Spectrom 1995;10:1–
3299 5.
186
3300 [208] Günther D, Longerich HP, Jackson SE, Forsythe L. Effect of sampler orifice
3301 diameter on dry plasma inductively coupled plasma mass spectrometry (ICP-MS)
3302 backgrounds, sensitivities, and limits of detection using laser ablation sample introduction.
3305 the aqua regia soluble content of rare earth elements in fertilizer, animal fodder phosphate
3306 and manure samples using inductively coupled plasma mass spectrometry. Anal Chim Acta
3307 1998;373:95–105.
3308 [210] Hevesy G, Levi H. Action of Slow Neutrons on Rare Earth Elements. Nature
3309 1936;137:185.
3310 [211] Greenberg RR, Mackey EA, Becker DA. Radioanalytical Methods : Data Quality ,
3311 Method Validation and Use of Standard Reference Materials ( continued )The application of
3312 instrumental neutron activation analysis for the certification of the new NIST fly ash SRM. J
3315 reference materials by instrumental neutron activation analysis. J Radioanal Nucl Chem
3317 [213] Smolka-Danielowska D. Rare earth elements in fly ashes created during the coal
3318 burning process in certain coal-fired power plants operating in Poland - Upper Silesian
3320 https://doi.org/10.1016/j.jenvrad.2010.07.001.
3321 [214] Gluskoter HJ, Ruch RR, Miller WG, Cahill RA, Dreher GB. Trace elements in coal:
3322 occurrence and distribution. Final report,June 1974--June 1976. Urbana, IL: Illinois State
3324 [215] Kuhn JK, Harfst WF, Shimp NF. X-ray fluorescence analysis of whole coal. Trace
3326 [216] Prather JW, Guin JA, Tarrer AR. X-ray fluorescence analysis of trace elements in
3327 coal and solvent refined coal. Energy & Fuels 1990;4:440–2.
3328 [217] Bettinelli M, Taina P. Rapid analysis of coal fly ash by x‐ray fluorescence
3331 XRF Spectroscopy as a Screening Tool for Rare Earth Elements in Coal and Coal Waste
3335 combustion ashes from selected Polish coal mines by wavelength dispersive X-ray
3337 https://doi.org/10.1016/j.sab.2015.12.005.
3338 [220] Chuparina E V., Chubarov VM, Paradina LP. A comparative determination of major
3339 components in coal power plant wastes by wavelength dispersive X-ray fluorescence using
3340 pellet and fused bead specimens. Appl Radiat Isot 2019;152:162.
3341 https://doi.org/10.1016/j.apradiso.2019.06.040.
3342 [221] Yang X, Kozar D, Gorski D, Marchese A, Pagnotti J, Sutterlin R, et al. Using yttrium
3343 as an indicator to estimate total rare earth element concentration: a case study of
3344 anthracite-associated clays from northeastern Pennsylvania. Int J Coal Sci Technol 2020.
3345 https://doi.org/10.1007/s40789-020-00316-1.
3346 [222] Hughes R, Barker SLL. Using portable XRF to infer adularia halos within the Waihi
3347 Au-Ag system, New Zealand. Geochemistry Explor Environ Anal 2018;18:97–108.
3348 [223] Richards MJ. Realising the potential of portable XRF for the geochemical
3350 [224] Higueras P, Oyarzun R, Iraizoz JM, Lorenzo S, Esbrí JM, Martínez-Coronado A.
3351 Low-cost geochemical surveys for environmental studies in developing countries: Testing a
3352 field portable XRF instrument under quasi-realistic conditions. J Geochemical Explor
3353 2012;113:3–12.
3354 [225] Carr R, Zhang C, Moles N, Harder M. Identification and mapping of heavy metal
3355 pollution in soils of a sports ground in Galway City, Ireland, using a portable XRF analyser
3357 [226] Melquiades FL, Appoloni C. Application of XRF and field portable XRF for
188
3359 [227] Kalnicky DJ, Singhvi R. Field portable XRF analysis of environmental samples. J
3361 [228] Kiss LT. X-Ray Fluorescence Determination of Brown Coal Inorganics. Anal Chem
3363 [229] Zhang W, Noble A, Yang X, Honaker R. A Comprehensive Review of Rare Earth
3365 [230] Liu P, Yang L, Wang Q, Wan B, Ma Q, Chen H, et al. Speciation transformation of
3366 rare earth elements (REEs) during heating and implications for REE behaviors during coal
3368 [231] Hower JC, Qian D, Briot NJ, Henke KR, Hood MM, Taggart RK, et al. Rare earth
3369 element associations in the Kentucky State University stoker ash. Int J Coal Geol
3371 [232] Stuckman MY, Lopano CL, Granite EJ. Distribution and speciation of rare earth
3372 elements in coal combustion by-products via synchrotron microscopy and spectroscopy. Int
3374 [233] Taggart RK, Rivera NA, Levard C, Ambrosi JP, Borschneck D, Hower JC, et al.
3375 Differences in bulk and microscale yttrium speciation in coal combustion fly ash. Environ
3377 [234] Zhang Z, Junming S, He Y, Liu G, Wang Y, Cao H. Distribution of some major and
3379 https://doi.org/10.1017/CBO9781107415324.004.
3380 [235] Hower JC, Groppo JG. Rare Earth-bearing particles in fly ash carbons: Examples
3381 from the combustion of eastern Kentucky coals. Energy Geosci 2020.
3382 https://doi.org/10.1016/j.engeos.2020.09.003.
3383 [236] Hower JC, Cantando E, Eble CF, Copley GC. Characterization of stoker ash from the
3384 combustion of high-lanthanide coal at a Kentucky bourbon distillery. Int J Coal Geol
3386 [237] Thompson RL, Bank T, Montross S, Roth E, Howard B, Verba C, et al. Analysis of
3387 rare earth elements in coal fly ash using laser ablation inductively coupled plasma mass
189
3388 spectrometry and scanning electron microscopy. Spectrochim Acta - Part B At Spectrosc
3390 [238] Hower J, Groppo J, Joshi P, Dai S, Moecher D, Johnston M. Location of Cerium in
3391 Coal-Combustion Fly Ashes: Implications for Recovery of Lanthanides. Coal Combust
3393 [239] Wirtz T, De Castro O, Audinot J-N, Philipp P. Imaging and analytics on the helium
3395 [240] Valley JW, Reinhard DA, Cavosie AJ, Ushikubo T, Lawrence DF, Larson DJ, et al.
3397 and SIMS: New tools for old minerals. Am Mineral 2015;100:1355–77.
3398 [241] Schmitt AK, Zack T. High-sensitivity U–Pb rutile dating by secondary ion mass
3399 spectrometry (SIMS) with an O2+ primary beam. Chem Geol 2012;332:65–73.
3400 [242] Horn I, Hinton RW, Jackson SE, Longerich HP. Ultra‐trace element analysis of
3401 NIST SRM 616 and 614 using laser ablation microprobe‐inductively coupled plasma‐mass
3404 [243] Wiese Jr RG, Muir IJ, Fyfe WS. Trace-element siting in iron sulfides in Ohio coals
3405 determined by secondary ion mass spectrometry (SIMS). Int J Coal Geol 1990;14:155–74.
3406 [244] Spears DA. The use of laser ablation inductively coupled plasma-mass spectrometry
3407 (LA ICP-MS) for the analysis of fly ash. Fuel 2004;83:1765–70.
3408 https://doi.org/10.1016/j.fuel.2004.02.018.
3409 [245] Bauer G, Achleitner B, Bonta M, Friedbacher G, Limbeck A. Analysis of single fly
3410 ash particles using laser ablation ICP-MS–an approach achieving lateral elemental
3412 [246] Kostova I, Vassileva C, Dai S, Hower JC. Mineralogy, geochemistry and mercury
3413 content characterization of fly ashes from the Maritza 3 and Varna thermoelectric power
3415 [247] Roth EA, Thompson RL, Lin R, Bank TL, Granite E. Distributions and Associations
3416 of Rare Earth Elements in Fly Ash Using Laser Ablation Sector Field ICP-MS. AICHE Natl.
3420 https://doi.org/10.1016/j.coal.2018.02.011.
3422 advances in quantitative LA-ICP-MS analysis: challenges and solutions in the life sciences
3424 [250] Mardon SM, Hower JC. Impact of coal properties on coal combustion by-product
3425 quality : examples from a Kentucky power plant. Int J Coal Geol 2004;59:153–69.
3426 https://doi.org/10.1016/j.coal.2004.01.004.
3427 [251] Hower JC, Groppo JG, Hsu-kim H, Taggart RK. Distribution of rare earth elements
3428 in fly ash derived from the combustion of Illinois Basin coals. Fuel 2021;289:119990.
3429 https://doi.org/10.1016/j.fuel.2020.119990.
3431 Multielements in High-Alumina Coal and Coal Ash: A Case Study of Datong Coalfield.
3434 and geochemistry of coal from the Liupanshui mining district, Guizhou, south China. Int J
3436 [254] Dai S, Zou J, Jiang Y, Ward CR, Wang X, Li T, et al. Mineralogical and geochemical
3437 compositions of the Pennsylvanian coal in the Adaohai Mine, Daqingshan Coalfield, Inner
3438 Mongolia, China: Modes of occurrence and origin of diaspore, gorceixite, and ammonian
3440 [255] American Coal Ash Association. Coal combustion products production and use
3442 [256] The 69th annual edition of the BP Statistical Review of World Energy.
3443 https://www.bp.com/content/dam/bp/business-sites/en/global/corporate/pdfs/energy-econo
191
3446 [257] Ding J, Ma S, Shen S, Xie Z, Zheng S, Zhang Y. Research and industrialization
3447 progress of recovering alumina from fly ash: A concise review. Waste Manag 2017;60:375–
3449 [258] Hower J, Groppo J, Jewell RF, Wiseman JD, Duvallet T, Oberlink A, et al.
3450 Distribution of Rare earth elements in the pilot-scale processing of fly ashes derived from
3451 eastern Kentucky coals Comparisons of the feed and processed ashes. Fuel 2021;in
3452 press:xxx–xxx.
3453 [259] Hower JC, Dai S, Seredin V V, Zhao L, Kostova IJ, Silva LFO, et al. A Note on the
3454 Occurrence of Yttrium and Rare Earth Elements in Coal Combustion Products. Coal
3456 [260] Piispanen MH, Arvilommi SA, Broeck B Van den, Nuutinen LH, Tiainen MS,
3457 Perä mä ki PJ, et al. A comparative study of fly ash characterization by LA-ICP-MS and
3459 [261] Chehreh Chelgani S, Hower JC. Estimating REY content of eastern Kentucky coal
3460 samples based on their associated ash elements. J Rare Earths 2018;36:1234–8.
3461 https://doi.org/10.1016/j.jre.2018.02.015.
3462 [262] Hower JC, Fu B, Dai S. Geochemical partitioning from pulverized coal to fly ash and
3464 [263] Hower JC, Groppo JG, Graham UM, Ward CR, Kostova IJ, Maroto-Valer MM, et al.
3465 Coal-derived unburned carbons in fly ash: A review. Int J Coal Geol 2017;179:11–27.
3466 https://doi.org/10.1016/j.coal.2017.05.007.
3467 [264] Hower JC, Groppo JG, Joshi P, Preda D V, Gamliel DP, Mohler DT, et al.
3468 Distribution of Lanthanides, Yttrium, and Scandium in the Pilot-Scale Beneficiation of Fly
3470 [265] Hower JC, Graham UM, Dozier A, Tseng MT, Khatri RA. Association of the sites of
3471 heavy metals with nanoscale carbon in a Kentucky electrostatic precipitator fly ash. Environ
3473 [266] Meij R. Trace element behavior in coal-fired power plants. Fuel Process Technol
192
3475 [267] Smith RD, Campbell JA, Felix WD. Atmospheric trace element pollutants from coal
3477 [268] Clarke LB. The fate of trace elements during coal combustion and gasification: an
3479 [269] Wang Z. Geochemistry of rare earth elements. Beijing: Science Press (Beijing);
3480 1989.
3481 [270] Yao DX, Zhi XC, Wang X. Geochemical feature and laws of concentrtion and
3482 dispersion of rare earth elements between coals and their fly asn bottom ashes. Geochemica
3484 [271] Fu B, Liu G, Sun M, Hower JC, Mian MM, Wu D, et al. Emission and
3485 transformation behavior of minerals and hazardous trace elements (HTEs) during coal
3487 https://doi.org/10.1016/j.envpol.2018.07.066.
3488 [272] Mardon SM, Hower JC, O’Keefe JMK, Marks MN, Hedges DH. Coal combustion
3489 by-product quality at two stoker boilers: Coal source vs. fly ash collection system design. Int
3493 [274] Cherniak DJ, Watson EB, Thomas JB. Diffusion of helium in zircon and apatite.
3495 [275] Farley KA. He diffusion systematics in minerals: Evidence from synthetic monazite
3497 [276] Zeitler PK, Herczeg AL, McDougall I, Honda M. U-Th-He dating of apatite: A
3501 [278] Tõnsuaadu K, Gross KA, Pluduma L, Veiderma M. A review on the thermal stability
3503 https://doi.org/10.1007/s10973-011-1877-y.
193
3504 [279] Senior C. Mercury behavior in coal combustion systems. John Wiley & Sons, Ltd.;
3505 2015.
3506 [280] Williams A, Pourkashanian M, Jones JM. Combustion of pulverised coal and
3508 https://doi.org/10.1016/S0360-1285(01)00004-1.
3509 [281] Xu M, Yan R, Zheng C, Qiao Y, Han J, Sheng C. Status of trace element emission in
3511 https://doi.org/10.1016/S0378-3820(03)00174-7.
3512 [282] Lyon RK, Freund H. Coal combustion process. US Pat 4,285,283 1981;4.
3513 https://doi.org/10.16533/j.cnki.15-1099/tf.2013.05.012.
3514 [283] Vassilev S V., Vassileva CG. A new approach for the classification of coal fly ashes
3515 based on their origin, composition, properties, and behaviour. Fuel 2007;86:1490–512.
3516 https://doi.org/10.1016/j.fuel.2006.11.020.
3517 [284] Hemmings RT, Berry EE. On the Glass in Coal Fly Ashes: Recent Advances. MRS
3519 [285] Ward CR, French D. Determination of glass content and estimation of glass
3520 composition in fly ash using quantitative X-ray diffractometry. Fuel 2006;85:2268–77.
3521 https://doi.org/10.1016/j.fuel.2005.12.026.
3522 [286] Henry J, Towler MR, Stanton KT, Querol X, Moreno N. Characterisation of the
3523 glass fraction of a selection of European coal fly ashes. J Chem Technol Biotechnol
3526 high-temperature melts of coal ashes and other silicates. Prog Energy Combust Sci
3529 Aluminosilicates in Fly Ashes with Different Melting Points Using 27Al Magic-Angel
3531 https://doi.org/10.1021/acs.energyfuels.7b01466.
194
3532 [289] Tian S, Zhuo Y, Chen C. Characterization of the products of the clay mineral thermal
3533 reactions during pulverization coal combustion in order to study the coal slagging
3535 [290] Towler MR, Stanton KT, Mooney P, Hill RG, Moreno N, Querol X. Modelling of
3536 the glass phase in fly ashes using network connectivity theory. J Chem Technol Biotechnol
3538 [291] San Nicolas RVR, Walkley B, van Deventer JSJ. Fly ash-based geopolymer
3539 chemistry and behavior. Coal Combust Prod Charact Util Benef 2017:185–214.
3540 https://doi.org/10.1016/B978-0-08-100945-1.00007-1.
3541 [292] Schwarz N, Cam H, Neithalath N. Influence of a fine glass powder on the durability
3542 characteristics of concrete and its comparison to fly ash. Cem Concr Compos 2008;30:486–
3544 [293] Shi C, Wu Y, Riefler C, Wang H. Characteristics and pozzolanic reactivity of glass
3546 [294] Yan J, Neretnieks I. Is the glass phase dissolution rate always a limiting factor in the
3548 https://doi.org/10.1016/0048-9697(95)04727-1.
3550 and Glass Products. Philadelphia, United States: ASTM International; 2004.
3551 [296] Jiang Z-H, Zhang Q-Y. The formation of glass: a quantitative perspective. Sci China
3553 [297] Hower JC, Henke KR, Dai S, Ward CR, French D, Liu S, et al. Coal Combustion
3554 Products (CCPs): Characteristics, Utilization and Beneficiation. Chapter 2: Generation and
3555 nature of coal fly ash and bottom ash. Elsevier Ltd.; 2017.
3556 https://doi.org/10.1016/B978-0-08-100945-1.00002-2.
3557 [298] Saikia BK, Hower JC, Hood MM, Baruah R, Dekaboruah HP, Boruah R, et al.
3558 Petrological and biological studies on some fly and bottom ashes collected at different times
3560 https://doi.org/10.1016/j.fuel.2015.06.007.
195
3561 [299] Hower JC. Petrographic examination of coal-combustion fly ash. Int J Coal Geol
3563 [300] Suárez-Ruiz I, Valentim B, Borrego AG, Bouzinos A, Flores D, Kalaitzidis S, et al.
3565 and co-combustion. (An ICCP Classification System, Fly-Ash Working Group –
3567 https://doi.org/10.1016/j.coal.2017.06.004.
3568 [301] Hower JC, Suárez-Ruiz I, Mastalerz M. An approach toward a combined scheme for
3569 the petrographic classification of fly ash: Revision and clarification. Energy and Fuels
3571 [302] Creelman RA, Ward CR, Schumacher G, Juniper L. Relation between coal mineral
3572 matter and deposit mineralogy in pulverized fuel furnaces. Energy and Fuels 2013;27:5714–
3574 [303] Zyrkowski M, Neto RC, Santos LF, Witkowski K. Characterization of fly-ash
3576 https://doi.org/10.1016/j.fuel.2016.01.061.
3577 [304] Wall TF, Creelman RA, Gupta RP, Gupta SK, Coin C, Lowe A. Coal ash fusion
3578 temperatures - New characterization techniques, and implications for slagging and fouling.
3580 https://doi.org/10.1016/S0360-1285(98)00010-0.
3581 [305] Brindle JH, McCarthy MJ. Chemical constraints on fly ash glass compositions.
3583 [306] Durdziński PT, Snellings R, Dunant CF, Haha M Ben, Scrivener KL. Fly ash as an
3585 https://doi.org/10.1016/j.cemconres.2015.08.005.
3586 [307] Srinivasachar S, Helble JJ, Boni AA. Mineral behavior during coal combustion1.
3588 [308] Srinivasachar S, Helble JJ, Boni AA, Shah N. Mineral behavior during coal
196
3590 [309] Helble JJ, Srinivasachar S, Boni AA. Factors influencing the transformation of
3591 minerals during pulverized coal combustion. Prog Energy Combust Sci 1990;16:267–79.
3592 https://doi.org/10.1016/0360-1285(90)90036-3.
3593 [310] Wigley F, Williamson J. Modelling fly ash generation for pulverised coal
3596 mineralogy, chemical speciation, and combustion behavior of toxic elements of coal
3598 [312] Vassilev S V., Vassileva CG. Occurrence, abundance and origin of minerals in coals
3600 https://doi.org/10.1016/S0378-3820(96)01021-1.
3601 [313] Osborn EF, Muan A, Levin EM, Robbins CM, McMurdie HF. Phase equilibrium
3602 diagrams of oxide systems. The system CaO-Al2O3-SiO2. Am Ceram Socicty 1960;15:6–
3603 63.
3604 [314] Alekseev YI, Vereshchagin VI. Formation of crystalline phases in electroceramics of
3605 the system CaO− MgO− Al 2 O 3− SiO 2 (A review). Glas Ceram 1997;54:340–3.
3606 [315] Fudali RF. The Interpretation of Geological Phase Diagrams. J Geol 1974;82:529–
3607 30.
3608 [316] Huffman GP, Huggins FE, Dunmyre GR. Investigation of the high-temperature
3609 behaviour of coal ash in reducing and oxidizing atmospheres. Fuel 1981;60:585–97.
3610 [317] Abbott MF, Austin LG. Studies on slag deposit formation in pulverized-coal
3611 combustors: 6. sticking behaviour of slag drops from three Pennsylvania steam coals. Fuel
3612 1985;64:832–8.
3614 https://doi.org/10.1016/j.fuel.2017.06.059.
3615 [319] Li Y, Gao X, Wu H. “Ash Cenosphere from Solid Fuels Combustion. Part 2:
3616 Significant Role of Ash Cenosphere Fragmentation in Ash and Particulate Matter Formation.
3618 [320] Kleinhans U, Wieland C, Frandsen FJ, Spliethoff H. Ash formation and deposition in
3619 coal and biomass fired combustion systems: Progress and challenges in the field of ash
197
3620 particle sticking and rebound behavior. Prog Energy Combust Sci 2018;68:65–168.
3621 https://doi.org/10.1016/j.pecs.2018.02.001.
3622 [321] Reinmöller M, Klinger M, Schreiner M, Gutte H. Relationship between ash fusion
3623 temperatures of ashes from hard coal, brown coal, and biomass and mineral phases under
3626 [322] Liu Y, Gupta R, Sharma A, Wall T, Butcher A, Miller G, et al. Mineral
3629 [323] Brown GEJ. X-ray scattering and X-ray spectroscopy studies of silicate melts. Struct
3631 [324] Zachariasen WH. The atomic arrangement in glass. J Am Chem Soc 1932;44.
3632 https://doi.org/10.1021/ja01349a006.
3633 [325] Fujita T, Konno K, Zhang W, Kumar V, Matsuura M, Inoue A, et al. Atomic-scale
3634 heterogeneity of a multicomponent bulk metallic glass with excellent glass forming ability.
3636 [326] Xi XK, Li LL, Zhang B, Wang WH, Wu Y. Correlation of atomic cluster symmetry
3637 and glass-forming ability of metallic glass. Phys Rev Lett 2007;99:95501.
3638 https://doi.org/10.1103/PhysRevLett.99.095501.
3639 [327] Keen DA, McGreevy RL. Structural modelling of glasses using reverse Monte Carlo
3641 [328] Hirata A, Guan P, Fujita T, Hirotsu Y, Inoue A, Yavari AR, et al. Direct observation
3643 https://doi.org/10.1038/nmat2897.
3644 [329] Miracle DB. A structural model for metallic glasses. Nat Mater 2004;3:697–702.
3645 https://doi.org/10.1038/nmat1219.
3646 [330] Bernal JD. Geometry of the Structure of Monatomic Liquids. Nature 1960;185:68–
3648 [331] Gaskell PH. A new structural model for transition metal-metalloid glasses. Nature
3651 combustion products from Kentucky power plants: Results from the 2007 sampling, with
3653 https://doi.org/10.4177/ccgp-d-09-00013.1.
3654 [333] Hower JC, Rimmer SM, Mastalerz M, Wagner NJ. Migmatite-like textures in
3655 anthracite : Further evidence for low-grade metamorphic melting and resolidification in
3657 [334] Kang SH. Fundamental Studies of Mineral Matter Transformation During
3660 [335] Lee Y. CCSEM analysis of minerals in pulverized coal and ash formation modelling.
3661 Ph. D. Thesis. Massachusetts Institute of Technology. Dept. of Chemical Engineering. 2000.
3662 [336] Padia A. The behavior of ash in pulverized coal under simulated combustion
3665 [337] Quann RJ, Sarofim AF. A scanning electron microscopy study of the
3666 transformations of organically bound metals during lignite combustion. Fuel 1986;65:40–6.
3667 [338] Ramsden AR. Microscopic investigation into the formation of fly-ash during the
3669 [339] Vejahati F, Xu Z, Gupta R. Trace elements in coal: Associations with coal and
3670 minerals and their behavior during coal utilization - A review. Fuel 2010;89:904–11.
3671 https://doi.org/10.1016/j.fuel.2009.06.013.
3672 [340] Wang H, Harb JN. Modeling of ash deposition in large-scale combustion facilities
3674 https://doi.org/10.1016/s0360-1285(97)00010-5.
3675 [341] Yan L, Gupta RP, Wall TF. The implication of mineral coalescence behaviour on ash
3676 formation and ash deposition during pulverised coal combustion. Fuel 2001;80:1333–40.
3677 https://doi.org/10.1016/S0016-2361(00)00194-0.
3678 [342] Brady JB, Cherniak DJ. Diffusion in minerals: an overview of published
3681 effects in a variety of crustal magma types. Earth Planet Sci Lett 1983;64:295–304.
3684 DFT Calculations: What Structural Factors Dictate the Chemical Shifts? J Phys Chem C
3686 [345] Jaworski A, Stevensson B, Edén M. The Bearings from Rare-Earth (RE = La, Lu, Sc,
3688 Solid-State 17O NMR, Molecular Dynamics Simulations, and DFT Calculations. J Phys
3691 2O3-Al2O3-SiO2 system and its subsystems. Calphad Comput Coupling Phase Diagrams
3693 [347] Wang X, Zhang R, Ren J, Vezin H, Fan S, Yu C, et al. Mechanism of cluster
3696 https://doi.org/10.1016/j.jallcom.2016.11.104.
3698 aluminosilicate glasses probed by molecular dynamics simulations. J Non Cryst Solids
3701 Melt properties, crystallization, and the network structures. J Non Cryst Solids
3703 [350] Florian P, Sadiki N, Massiot D, Coutures JP. 27Al NMR study of the structure of
3704 lanthanum- And yttrium-based aluminosilicate glasses and melts. J Phys Chem B
3706 [351] Zheng Q, Smedskjaer MM, Youngman RE, Potuzak M, Mauro JC, Yue Y. Influence
200
3709 [352] Pahari B, Iftekhar S, Jaworski A, Okhotnikov K, Jansson K, Stevensson B, et al.
3711 by multinuclear 45 Sc, 27 Al, and 29 Si solid-state NMR. J Am Ceram Soc 2012;95:2545–
3714 mixed rare earth minerals calcined by CaO-NaCl-CaCl2. Trans Nonferrous Met Soc China
3717 glasses. I. The structural role of La3+ cations. J Non Cryst Solids 2002;297:220–38.
3718 https://doi.org/10.1016/S0022-3093(01)00935-8.
3719 [355] Pohlenz J, Rosa AD, Mathon O, Pascarelli S, Belin S, Landrot G, et al. Structural
3722 https://doi.org/10.1016/j.chemgeo.2017.12.023.
3724 Properties and structures of RE2O3-Al 2O3-SiO2 (RE = Y, Lu) glasses probed by molecular
3725 dynamics simulations and solid-state NMR: The roles of aluminum and rare-earth ions for
3727 https://doi.org/10.1021/jp302672b.
3728 [357] Pozdnyakova I, Sadiki N, Hennet L, Cristiglio V, Bytchkov A, Cuello GJ, et al.
3729 Structures of lanthanum and yttrium aluminosilicate glasses determined by X-ray and
3731 https://doi.org/10.1016/j.jnoncrysol.2007.11.012.
3732 [358] Jaworski A, Stevensson B, Pahari B, Okhotnikov K, Eden M. Local structures and
3733 Al/Si ordering in lanthanum aluminosilicate glasses explored by advanced 27Al NMR
3734 experiments and molecular dynamics simulations. Phys Chem Chem Phys 2012;14:15866–
3735 78.
3736 [359] Okhotnikov K, Stevensson B, Edén M. New interatomic potential parameters for
3737 molecular dynamics simulations of rare-earth (RE= La, Y, Lu, Sc) aluminosilicate glass
201
3738 structures: exploration of RE 3+ field-strength effects. Phys Chem Chem Phys
3739 2013;15:15041–55.
3740 [360] Wang MT, Cheng JS, Li M, He F. Structure and properties of soda lime silicate glass
3742 https://doi.org/10.1016/j.physb.2010.10.040.
3743 [361] Wang M, Cheng J, Liu Q, Tian P, Li M. The effect of light rare earths on the
3746 [362] Bois L, Barré N, Guillopé S, Guittet MJ, Gautier-Soyer M, Duraud JP, et al.
3748 https://doi.org/10.1016/S0022-3115(99)00137-3.
3749 [363] Zhang W, Groppo J, Honaker R. Ash beneficiation for REE recovery. 2015 World
3751 [364] King JF, Taggart RK, Smith RC, Hower JC, Hsu-Kim H. Aqueous acid and alkaline
3752 extraction of rare earth elements from coal combustion ash. Int J Coal Geol 2018;195:75–83.
3753 https://doi.org/10.1016/j.coal.2018.05.009.
3755 Elements from Coal Fly Ash Particles in a Dilute H2SO4 Solvent. Open J Phys Chem
3757 [366] Pan J, Hassas BV, Rezaee M, Zhou C, Pisupati S. Recovery of rare earth elements
3758 from coal fly ash thorugh sequential chemical roasting, water leaching, and acid leaching
3760 https://doi.org/https://doi.org/10.1016/j.jclepro.2020.124725.
3761 [367] Huang C, Wang Y, Huang B, Dong Y, Sun X. The recovery of rare earth elements
3762 from coal combustion products by ionic liquids. Miner Eng 2019;130:142–7.
3763 https://doi.org/10.1016/j.mineng.2018.10.002.
3764 [368] Nayaka GP, Zhang Y, Dong P, Wang D, Zhou Z, Duan J, et al. An environmental
3765 friendly attempt to recycle the spent Li-ion battery cathode through organic acid leaching. J
202
3767 [369] Wen Z, Zhou C, Pan J, Cao S, Hu T, Ji W, et al. Recovery of rare-earth elements
3768 from coal fly ash via enhanced leaching. Int J Coal Prep Util 2020:1–15.
3769 https://doi.org/10.1080/19392699.2020.1790537.
3772 https://doi.org/10.1016/S0304-386X(00)00146-8.
3774 Aqueous Sodium Hydroxide Solutions at High Pressure and Temperature. Can J Chem Eng
3776 [372] Kumari A, Panda R, Jha MK, Kumar JR, Lee JY. Process development to recover
3777 rare earth metals from monazite mineral: A review. Miner Eng 2015;79:102–15.
3778 https://doi.org/10.1016/j.mineng.2015.05.003.
3779 [373] Peterson R, Heinrichs M, Argumedo D, Taha R. Recovery of rare earth elements
3780 from coal and coal byproducts via a closed loop leaching process : Final Report. 2017.
3781 https://doi.org/10.2172/1377818.
3782 [374] Cao DZ, Selic E, Herbell JD. Utilization of fly ash from coal-fired power plants in
3784 [375] Querol X, Moreno N, Umaa JC, Alastuey A, Hernández E, López-Soler A, et al.
3785 Synthesis of zeolites from coal fly ash: an overview. Int J Coal Geol 2002;50:413–23.
3786 https://doi.org/10.1016/S0166-5162(02)00124-6.
3788 and rare earth elements in rocks by high resolution inductively coupled plasma-mass
3790 https://doi.org/10.1111/j.1751-908X.1999.tb00557.x.
3794
3795
203