Surface Mine Blasting Techniques
Surface Mine Blasting Techniques
Airblast Instrumentation
and Measurement Techniques
for Surface Mine Blasting
US Department of Interior
Office of Surface Mining
Reclamation and Enforcement
Kenneth K. Eltschlager
Mining/Blasting Engineer
3 Parkway Center •
Pittsburgh, PA 15220
Phone 412.937.2169
Fax 412.937.3012
Keltschl@osmre.gov
Stachura, Virgil .J
Airblast instrumentation and measurement techniques for
surface mine blasting.
II:.LUSTRATIONS
ILLUSTRATIONS--Continued
TABLES
by
ABSTRACT
INTRODUCTION
Geophysicist.
2Electrical engineer.
All authors are with the Twin Cities Research Center, Bureau of Mines, Twin
Cities, Minn.
3 Underlined numbers in parentheses refer to items in the list of references
preceding the appendixes.
2
Some of the sources of airblast can be seen in figure 1. The white plume
just left of center is the source of stemming release pulses. To the right of
center, a hole has "cratered," transmitting more energy into the atmosphere
than into breaking rock. These gas releases, combined with the stress wave
energy transmitted from the rock and the heaving motion around the collar,
contribute to the higher frequency portion of airblast. A general swelling of
the shot area, including the free face, produces the "piston effect," a low-
frequency component of airblast. The high-frequency component is generally
above 5 to 6Hz, while the low-frequency portion is in the 0.5-to-2-Hz region
(28). The phenomenon of airblast generation has been studied extensively by
fifiss (39) and by Snell and Oltmans (33).
10.00
.100
1.00
.010
(\J
c:
.c
'
.c
...
E
.100 w...
w .001 a::
0::: :::::>
:::::> (/)
(/) (/)
(/) w
w a::
.010 a..
0:.::
a.. 10- 4 a::
0:.:: w
LLJ >
>
0
0
.001
10- 5
10- 5
1o- 7 ~~~~~~~~~~~~~~~~~~~~~
which is less than 15 dB below the low-frequency energy level. The Type I
airblast is more troublesome because of its energy in the resonant frequency
range of structures (28). Efforts to document the environmental effects of
this acoustic energy require highly specialized instrumentation, which takes
into account the frequencies and amplitudes generated by the source.
In this report, sound pressure levels are expressed in decibels and over-
pressures in pounds per square inch (psi). Other units used in acoustics are
millibars and Newtons per square meter (N/m 2 ), also known as Pascals (Pa).
Sonic boom levels are often expressed in units of pounds per square foot
(psf). A conversion chart is shown in figure 2. The two overpressure scales
are slightly offset and not symmetrical.
ACKNOWLEDGMENTS
PREVIOUS INVESTIGATIONS
The main transient noise sources that cause annoyance and damage are
sonic booms, surface blasts, artillery, explosive testing, nuclear blast simu-
lation, accidental explosions, and partially confined blasts (mining,
5
Kryter (18) examined sonic boom effects on structures based on peak over-
pressure levels, and also determined severity equivalencies between peak over-
pressures and "perceived noise levels" (Lpn• also labeled PNdb) from subsonic
jets. Lpn levels are rms values calculated from the "noy" values of highest
noise level in each octave (1/3 octave) band. The noy was derived from judg-
ment tests of perceived loudness conducted in a laboratory. Noy values cannot
be directly measured, so Schomer (27) described their involved calculations.
A later study by Kryter (19) involved a more complex "effective perceived
noise level" (Lepn) based-on the largest Lpn calculated from band measurements
every 0.5 sec, including a tone correction for turbine whine. Schomer (27)
summarized Kryter's studies and also proposed "composite noise ratings" (eNR),
a 24-hour integration with a 10-dB nighttime penalty. Schomer stated that the
fear of property damage is related to complaints, both of which are different
from psychological annoyance. The distinction is significant for the mining
industry.
NA Equivalent
sound level.
LAeq = 10 log1r T c [!It.
10LpA(t)/10dt-J
Running time average;
any time duration
where can be used; good
LAeq = A-weighted equivalent sound level for long-term noise
T = Time interval for average impact analysis.
LpA = A-weighted sound level during
time T (any weighting can be nsed)
>(a4oo) [L-A(t)+l0]/10 }
+
J>(aaoo) 10 " dt
Alternate form:
LAB • lO loglO -
1
to tl
t.,
J
1 (t)/lO
10 pA dt
where
LpA • A-weighted sound level during time
interval t 1 to t., (any weighting
can be used) r:,
NA PLdB Perceived PLdll • 55 + 20 log10 T p Developed to charac-
level, dB. terize the sharpness
where and loudness of
6P = Pressure change, psi sonic booms ..
T ~ Rise time sec. corresponding t()_::A:..P_ _ _ __, ___________~
NA Not available.
7
The CHABA Committee Report presents a summary of averaging and SEL meas-
urernent methods, including average sound level (Leq or LT), which runs aver-
ages over any desired time periods, and day-night average (Ldn), which is a
24-hour Leq with a 10-dB nighttime penalty. Schomer (25) also uses Ldn,
except that he introduces C-weighting. Both Schomer (25) and The CHABA Report
(36) examine LeE and LAE and relate them to annoyance potential of blasts.
Generally, the sources used to develop these levels--steady state (aircraft),
sonic booms, and unconfined surface blasts--are quite different from mine pro-
duction blasts. In particular, Schomer's (25) comparisons of artillery LAE's
to blasting do not consider the vast difference between amounts of A-weighted
energy present in the two sources. A more serious problem is the tendency to
include transients such as blasts in long-term (that is, 24-hr) sound aver-
ages which leads to anamalous situations where the relatively coarse Ldn
values do not accurately characterize the annoyance and damage potential of
infrequent events.
The Bureau (31) recently serveyed these noise descriptors and their
applicability to blasting, specifically comparing LeE's, special weightings,
and various linear sound levels with actual structure responses.
SOUND MEASUREMENT
Instrumentation
4Reference to specific brand names is made for identification only and does
not imply endorsement by the Bureau of Mines.
8
and < time constant, (sec), for any given pressure P0 to drop to (1/e) P 0
(see • 5),
frequency, but temperature expansion and contraction of the sealed air volume
and barometric pressure changes could damage the diaphragm and cause
drift (29).
The frequency response selected for airblast measurement may meet one of
several criteria. One rule-of-thumb is that gages should respond to four
times the frequency of interest (24). Using this rule, previously measured
airblasts (28, 31-32, 35, 39) suggest a range of 0.1 to 200Hz. Reed defined
a second criterion-ror~he~igh-frequency response based on attenuation of
Po
w
0:::
~
(j)
(j) T= time constant
w
0:::
0...
.Lpo
w 2
>
1-
<(
GJ ..!.. Po-
o::: e
0 2 3 4 5 6 7 8 9 10
T TIME, sec
FIGURE 5. - Relationship between time constant and relative pressure.
11
explosion waves from unconfined high explosive and nuclear blasts. He stated
that there appeared to be no need for greater response greater that 1 kHz,
except at locations very close to small explosions. For environmental moni-
toring at levels of 114 to 144 dB at distances greater than a kilometer, 1 kHz
would be adequate, if not an order of magnitude on the conservative side (24).
Confined mine production blasts would not generate the high frequencies Reed
observed. A third criterion is based on a theoretical study of Crocker and
Sutherland, which resulted in formulas and curves for calculating upper and
lower limits of frequency response (6). For ±10 pet accuracy in peak pressure
and positive phase durations, a range of 0.05 Hz to 1 kHz would be required.
The first criterion would be sufficient for confined mine production blasts,
while unconfined surface blasts would be best measured under the second and
third.
FM Tape Recorders
SLM's have selectable response times: slow, fast, impulse, and peak.
Slow, fast, and impulse have time constants of 1,000, 125, and 35 msec,
respectively (1-2). Peak response does not have a standardized time constant
but should be about 10 ~sec for rise times in the upper audio range. Storage
of the highest peak value is an important feature (peak hold) when measuring a
short, unexpected event.
Slow response is used to measure a random noise source, since its averag-
ing effect makes reading easier. Fast response has the same effect, but to a
lesser degree. Slow and fast produce rms readings only. Impulse response was
designed for short-duration, single-pulse events. The 35-msec integration is
based on the mean averaging time of the human ear. This setting should not be
used for correlation with structure response or damage, because the response
of the ear and structures are not related. The impulse setting has a 3-sec
decay time constant, which can introduce errors from successive pulses such as
those found in a delayed mine blast (~).
+10
0
OJ
"0 -10
w
0-20
::::>
1--
::i -30
a..
:E -40
<t:
-50
-60
-7o~~--~~~~--~~~~~--~~~~~--~~~~~~~~~~~
The most important features on SLM's for blast measurement are linear or
flat-peak mode of operation, C-slow mode of operation for approximating sound
exposure level, and peak-hold or sample-hold to retain the highest reading.
Wind blowing across a microphone can generate turbulence, which can cause
a noise measurement to be erroneously high. Figure 10 shows typical wind
6
0
(I) - 2
"0
w
(/) 4
z
0
a.. - 6
(/)
w
0: 8
w
> -10
1- KEY
<(
_J
w 12 2 Hz lower limit 10Hz lower limit
0:
-14
- - - - l-in. microphone ------I- in. microphone
- - - - lt2 in. microphone in. microphone
- - - - - 1t2
16 ----Direct -----Direct
5 10 20 50 100
FREQUENCY, Hz
II 0
ro
-.:::100
..J
w
>
w
..J
0
z
::J 90
0
(J)
KEY
a Wind parallel to diaphragm
80 b Wind perpendicular to diaphragm
cAs b with windscreen
d As a with windscreen
d
70~----~------~------~------~------~------~------~------~
0 10 20 30 40 50 60 70 80
WIND SPEED, mph
FIGURE 10. - Wind noise as function of wind speed in the range of 20Hz to 20 kHz Q).
noise for microphones with and without windscreens (3). For example, a wind
about 25 mph parallel to the diaphragm (a and d) gen;rated about 99 dB without
a windscreen and 73 dB with one. The windscreen reduced this noise by 26 dB.
Figure 11 illustrates the effects of wind perpendicular to the diaphragm
with and without a windscreen (23). The windscreen reduces wind noise by 17
to 28 dB in the 25 to 6,000 Hz range. The microphone should be protected from
direct exposure to wind; if not possible, a windscreen should be used.
The "change of height" method can determine the -3 dB response point with
the equation on page 9 and the dynamic calibration can be determined by the
following equation:
17
(T + 273)
h = PC 4.548 P0
T = temperature ( 0 c)
The calibration and comparison tests in this section were used to deter-
mine the most effective instrument and measurement technique for surface mine
blasting. A comparison of C-slow and CSEL normalized to 1.0 sec is presented
in figure 15. Standard commercial SLM's were used to obtain the C-slow
117
3
0
(/)
I
(.)
~
__J
w
> Ill
w
__J
0
z
:::)
0
(/)
105
99
93
87
87 93 99 I05 I II 117
SOUND LEVEL, CSEL, normalized to 1.0 sec
FIGURE 15. • C-Siow compared with CSEL, normalized to 1 sec.
21
KEY
10 - - B 8. K 2631 l-in. microphone
--Dallas Instruments AR-2 11;8 -in. microphone
co 5 ----- B 8. K 22091;2-in. microphone, 10-Hz lower limit
"0
- - - VME noisetector (prototype)
~ 0
=>
1--
__J -5
a..
~
<(- 10
-15
-20 L--~--L~-~~LUL__~-~-L~~_u~--~~-~-L~~---L-~~~~~
0.01 0.1 1.0 10.0 100.0
FREQUENCY, Hz
FIGURE 16.- Frequency response: B&K 2631, B~K 2209, Dallas Instruments AR-2, and
VME Noisetector.
15
10
co 5
"0
w
0 0 .... --------
,/"
...- -;/ ....-~-
L:
=> /
I- /
/ -""/
-5 KEY
/ "
__J I /
I
a.. I
/
/
/
~ 1;2 -in. microphone I
<( -10 I
I /
--Safeguard seismic unit Il ' /
-15 ----B 8. K 2209 l-in. microphone,2-Hz lower limit
---B e. K 2209 1-in.microphone,IO-Hz lower limit
-20
0.01 0.1 1.0 10.0 100.0
FREQUENCY, Hz
FIGURE 17.- Frequency response: B&K. 2631, B&K 2209, and Safeguard Seismic Unit II.
10 KEY
- - - GR 1933 1;2 -in. and l-in. electret microphone
ID 5 and l-in. ceramic microphone ·
"0
- - GRI551-C with impact analyzer
~ 0
----- VME Model F with l-in. ceramic
~- -- ----./-=::-::--::::-:::::-;:;.-=~------1
=> I , -
1-- microphone I 1/ //
...J -5 / I /
a.. --- B 8. K 2209 1;2 -in. microphone, 2-Hz I I I
:::E lower limit
<( -10 / I
-15
-20
0.01 0.1 1.6 10.0 100.0
FREQUENCY, Hz
FIGURE 18.- Frequency response: GR 1933, GR 1551-C, VME Model F, and B&K 2209.
22
readings, and a GR-1926 rms detector was used for the CSEL values. The corre-
lation coefficient of C-slow versus CSEL is 0.986, and standard deviation is
0.0000628 psi with a best-fit line of Y ~ 0.968 X+ 0.0000169 psi. Individual
data points are listed in table B-1. The high degree of correlation suggests
that C-slow may be an approximation for shots of 1.0-sec duration or less.
Longer shots require an SLM modified to integrate for longer than 1.0 sec or
the correction factors given by Kamperman. His corrections for shots of 0.5,
1.0, and 2.0 sec were 1, 2, and 3.5 dB, respectively (~).
~ 0
::J
t-
::i - 5
Q_
2
DP-7 transducer
//
,//
./' -- _...-------
/
/
<1-10 // /
DP-7 No. 10
133 dB peok,O.I-Hz cutoff (-3dB)
B 8 K 2209 linear
128 dB peak, 2-Hz cutoff (-3dB)
-----~
GR 1933 linear
~~~~~~---~-~~~--=-125dB peok,_?-Hz cutoff (-~dB)
B 8 K 2209 C-weighted
85-13c_ _ _-;Jl 111AMI.I>A!\M-.N""V1IV.kJ Mw-v..._.~-~~--~-------12Q~_I?~~k,_~5j:l3__~utof!__{-3d8)
C-slow meter reading
0 0.5 109 dB C
I""'P""""""""''"""liiiiiiil"!!"""liiiiiil,..........,~
TIME, sec
FIGURE 20. · Type I airblast measured four different ways.
23
-10
-30
-40
-50
-10
CD
"0
~ -20 2-Hz, linear-peak
w
a
::J
1- -30
_J
0..
:! -40
<{
w
> -50
1-
<{
_J -20
w 5-Hz, linear-peak
0::
-30
-40
-50
-20
C-weighted-peak
-30
-40
-50
-60
0 10 20 30 40 50
FREQUENCY, Hz
DP-7 No.8
48-13 I 21 dB peak,O. 1-Hz cutoff (-3 dB)
B a K 2209 linear
I 19 dB peak, 2-Hz cutoff (-3d B)
~
GR I933 linear
Ill dB peok,5·Hz cutoff (-3dB)
~~~
GR 1933 C-weighted
48-13c 99 dB peok,31.5·Hz cutoff (-3dB)
--~~~NW~~~~~~~--------------~---~~~-
0 0.5 C-SIOW meter reading
~ 85 lt2 dBC
TIME, sec
A typical Type I coal mine highwall shot is shown in figure 20. The 2-Hz
instrument reads 5 dB low and shows a shift in peak value to the right and
below the center line because of "ringing." This ringing causes a reduction
in amplitude and a phase shift due to the instrument's inability to follow the
lower frequency excursions of the airblast. The 5-Hz and C-weighted instru-
ments show further reductions in amplitude of 8 and 13 dB, respectively, with
a C-slow meter reading 24 dB below the most linear instrument. The frequency
spectra for figure 20 are shown in figure 21. This further illustrates the
loss of amplitude at lower frequencies.
The 2-Hz instrument has its response least affected for both types of
airblast, since the 1-Hz energy is so close to the -3 dB point. The response
of the 5-Hz and C-weighted instruments sharply decreases (a lower reading for
the same airblast) for the Type II blasts because of the absence of higher
frequency energy. The 2-Hz instrument gives a more accurate measure of the
total energy in an airblast than the 5-Hz or C-weighted instruments.
Shake table tests were run on the Validyne DP-7 to determine the effects
of vibration at a constant peak acceleration. A comparison with the DP-7 can
be made to a standard B&K 2209, with a l-inch microphone (fig. 24). The level
generated by external vibration ranges from 68 to 73 dB at a constant sinusoi-
dal acceleration of 1 g. An additional test was made to determine the effect
of air being driven into the open port of the transducer. A relatively low
level of noise (58 to 63 dB) was generated at a high level of acceleration
(16 g). Vibration effects were minimal.
25
-10
0.1-H z, I in eo r-peak
-20
-30
-40
-50
-10
CD
-o
20
w
Cl
:::>
1- -30
..J
a..
:::iE -40
<t
w -50
>
1-
<t
..J
w
c:: -10
-20
-30
-40
-50
C-weig hted-peok
-30
-40
-50
0 10 20 30 40 50
FREQUENCY, Hz
FIGURE 23.- Spectra of Type II airblast measured four different
ways.
26
100
95
B & K 2209
90
~--a. .... ....
85
KEY
o Vertical motion perpendicular to diaphragm (a lg)
80 o Horizontal motion perpendicular to diaphragm (a= lg)
r:D e:. Air port pointed in, in direction of motion
-o
r {a=l6g) diaphragm parallel to motion
:::£ 75
<!
w
(L
70
65
60
55 ~
50
2 4 7 10 20 40 70 100
FREQUENCY, Hz
FIGURE 24. - Vibration response of DP-7 sound measurement transducer.
135
130
125
120
CD
"
-'
w 115
>
lU
-'
0
z
::;)
110
0
(/)
105
100
95
90 95 100 105 110 115 120 125 130 135 140 145 150
SOUND LEVEL, decibels measured with 0.1-Hz low-frequency cutoff
135
130
125
..,
Ol
..J
w 115
>
w
_)
0
:z II 0
:::>
0
(/)
105
100
95
90 95 100 105 110 115 120 125 130 135 140 145 150
SOUND LEVEL, decibels measured with Q.I-Hz low-frequency cutoff
140
135
130
125
120
.,m
_j
w 115
>
w
-'
Cl
3110
0
(/)
105
100
95
90 95 100 105 110 115 120 125 130 135 140 145 150
SOUND LEVEL, decibels measured with 0.1-Hz low-frequency cutoff
135
130
125
120
d> 115
w
-'
Cl
z 110
::>
0
(/)
105
,.
100
95
90 95 100 105 110 115 120 125 130 135 140 145 150
SOUND LEVEL, decibels measured with 0.1-Hz low-frequency cutoff
135
130
125
120
-'
~ 115
w
-'
0
2 110
::J
Sl
105
100
95
90 95 100 105 110 115 120 125 130 135 140 145 150
SOUND LEVEL, decibels measured with 0.1-Hz low-frequency cutoff
135
130
125
120
II)
'0
_;
~ 115
w
-'
0
3 II 0
Sl
105
100
95
90 95 100 105 110 115 120 125 130 135 140 145 150
SOUND LEVEL, decibels measured with 0.1-Hz low-frequency cutoff
The various shots are classified by the kind of mine; the coal mine shots
are broken down into three types. Highwall coal shots have a full or partial
free face but are well confined, since the overburden is not extensively dis-
placed. Parting shots are in the thin, hard material separating two coal
seams and are difficult to confine well. The assorted shots included ditch
and "sweetner" shots, which employed relatively shallow blast holes. "Sweet-
ner" shots were used to break up the overburden sufficiently to level the sur-
face for a walking dragline. All quarry blasts were in limestone. Metal mine
blasts were recorded at iron mines on Minnesota's Mesabi Iron Range; these
were very large and were recorded at greater distances than the coal or quarry
blasts.
Parting shots are very strong Type I blasts and show consistently higher
readings for 2-Hz, 5-Hz, C-slow, and PL dB methods. Metal mine shots at large
distances are strongly Type II, hence the 2-Hz, 5-Hz, C-slow, and PL dB meth-
ods are consistently lower. The selection of an instrument to measure Type I
blasts does not appear to be so critical as for Type II blasts, since 2-Hz and
5-Hz instruments read very nearly the same as 0.1-Hz instruments when measur-
ing parting shots. Generally, the standard deviations are smallest for the
2-Hz and 5-Hz instruments with two exceptions: coal mine parting and quarry
shots. These two exceptions are characterized by poorer confinement and the
heaving of material. Coal mines and quarries are often close to residences
and, therefore, reduce the chance of dispersing their high-frequency energy.
Any sound level meter used should be a Type I, impulse, precision instru-
ment. This type of meter is preferred because of its higher crest factor. A
peak "hold" feature is recommended when one is monitoring a short, unexpected
event. A C-slow reading may be obtained with such meters that have "true" or
"quasi" rms detectors with equal accuracy for blast measurements. The C-
weighting should meet ANSI 81.4-1971 specifications for Type I meter.
Production blasts are confined and delayed such that they generate a
lower band of frequencies than do open-air, single charges. Even when a hole
craters or blows out, confinement is enough to prevent the fast pressure rise
times seen in open airblasts. The distances at which production blasts are
monitored also reduce high frequencies through attenuation and dispersion. An
upper frequency of 200 Hz is sufficient for regulatory monitoring. For air-
blasts generated by mine production blasting, the frequency response should
meet or exceed the following specifications:
The 5-Hz and 6-Hz rolloff instruments will read essentially alike, so for
practical purposes they are interchangeable. For unconfined surface blasts at
short distances, an upper limit of 450 Hz or higher is recommended. For exam-
ple, uncovered detonating cord requires an extended high-frequency response.
For research tests, the lower limit should meet or exceed 0.1 Hz. A sound
level calibrator or pistonphone should be used to verify dynamic calibration
before each use. This calibrator should be checked anually against a source
traceable to the National Bureau of Standards.
A microphone windscreen will prevent false readings from wind gusts and
protect the microphone from shock damage or adverse weather. Foreign matter
could shift the frequency response by blocking the pressure equalization hole.
Microphones with a very low frequency response are more sensitive to wind
than those used for voice communication. The microphones should be on a tri-
pod or held motionless during a measurement, because variations in altitude
register as air pressure changes. The microphone should be at least 3 feet
aboveground and to the side of a structure to minimize reflections. The ori-
entation of the microphone is of minor importance, since it is directional
only at high frequencies (above 1,000 Hz) and essentially omnidirectional at
blast-generated frequencies.
REFERENCES
5. Bruel and Kjaer Instruments, Inc. Impulse Precision Sound Level Meter,
Type 2209. June 1972, 114 pp.
29. Siskind, D. E., and V. J. Stachura. Recording System for Blast Noise
Measurement. Sound and Vibration, June 1977, pp. 20-23.
32. Siskind, D. E., and C. R. Summers. Blast Noise Standards and Instrumen-
tation. BuMines TPR 78, 1974, 18 pp.
34. Sound and Vibration. S&V News. V. 12, No. 20, October 1978.
Shot 23/10 (fig. A-1).--A very strong type I airblast that illustrates
the presence of energy of up to 35 Hz at which point it is only 20 dB below
the peak value. The blast has a very fast pressure rise time, with one peak
predominating because of a clay seam that had been loaded through. This is a
quarry blast on a 95-ft face with four holes each containing a long and short
deck.
-----
0 0,5
TIME, sec
23/10
0
----- 0.5
60 ~~--~--~~-.~
Shot 23/10 50 Shot 2 7/7
40
30
20
10
~-L~QWWU~~~
20 40 60 80 100 0 20 40 60 80 100
FREQUENCY, Hz FREQUENCY, Hz
FIGURE A-1. - Quarry shots, 95-ft highwall: Type I airblast (shot 23/10) and reflected Type
II airblast (shot 27 /7).
Shots 31/1, 31/2, 31/3, 31/4 (fig. A-2).--In these time histories, a
quarry blast of two rows of 10 holes each was instrumented at four locations.
The direction of initiation was down the free face and toward the gage loca-
tion 31/1, with gage 31/3 located in the opposite direction. Gage 31/2 was
behind the shot on the top of the bench, and gage 31/4 was in front on the pit
bottom.
Shots 31/1 and 31/3 are similar in character except that the former
appears to be a time-compressed version of the other. This happens because
each successive borehole is closer to the gage station, shortening the travel
time and compressing the delay intervals. This also appears in the spectra as
a corresponding change in frequency content. Shot 31/1 has more energy above
20 Hz, while 31/3 continues to drop off gradually. Directing the initiation
away from a structure could change the frequency content sufficiently to
reduce problems.
In Shot 31/4, the individual pulses from the 10 front holes occur in 30-
to 45-msec intervals. This corresponds to the energy present in the spectra
37
0 0.5
Tl ME, sec
0 0.5
TIME, sec
~~
~~~~ 0.5
at 22 to 35 Hz, which is only about 12 dB down from the peak. There is more
mixing of pressure pulses in shot 31/2 than in shot 31/4 because of the prox-
imity of the second row of holes and the absence of a direct free face. More
energy is directed upward rather than back toward the gage. The energy in the
22- to 35-Hz range for shot 31/2 is 20 dB or more below the peak value, in
contrast to that in shot 31/4.
Shot 35/9 (fig. A-3).--This is a very long iron mine blast of 507,000
pounds of explosives, with a total of 147 delays in 148 holes. The distance
to the gage station was about 3,400 ft, and the shot duration was about 3.1
sec.The spectra shows a 22-Hz peak that is only 20 dB below the low-frequency
peak.
Shot 84/14 (fig. A-3).--This is a highwall coal mining shot with large
blast holes (15.5 in) monitored at about 750 ft. The first arrival is the
vertical motion of the ground near the microphone, since ground vibration
travels faster than airblast. The airblast arrived about 650 msec later and
showed the much sharper gas and stemming release pulses. Even though the time
0 0.5
TIME, sec
0 0.5
TIME, sec
0
----- TIME. sec
0.5
101-1
~ 60 r--1..........,.--,--,--,--.---~.,--,---,
l
~.~
;::: 50 Shot 35/9 60
::::; 40
Q
::;; 30
<l: 20 .
~ 10 ~~~~~~~~~_j 10 20 30 40 50
5
w
0 20 40 60 80 100 FREQUENCY, Hz
a:: FREQUENCY, Hz
FIGURE A-3. - Metal mine shot, very long duration oirblast (shot 35/9); coal mine shot, Type
II airblast, Iorge holes (shot 84/14); and coal mine shot, long-duration airblast,
six decks (shot 101/1).
39
history shows many sharp spikes, the frequency spectra indicate a continual
drop in energy to about 5 Hz, owing to the randomness of the gas and stemming
release pulses that prevented a buildup of energy at any particular frequency.
Shot 101/1 (fig. A-3).--In this shot the top decks were probably 60 msec
apart, which generated a large amount of energy at 17Hz, about 13 dB below
the peak value. The relatively uniform series of pulses caused the energy to
build at ·this frequency and shook the house at this site strongly.
Shot 105/7 (fig. A-4).--A reflection is obvious about 730 msec after the
first airblast arrival in this quarry shot. This "echo"contains energy in the
18-to 22-Hz region and shows up strongly in the spectra about 12 dB below the
peak. The house at this location responded more to the second airblast
because of its frequency content.
0 0.5
TIME, sec
0 0.5
Tl ME, sec
126/7
0 0.5
TIME, sec
147/7
60 ~~~~~~~~~
60 ~~~~~~~~~
50 50 Shot 147/7
Shot 105/7
40 40
30 30
20 20
10 10
20 40 60 80 I 00 0 40 80 120 160 200 0 20 40 60 80 100
FREQUENCY, dB FREQUENCY, Hz FREQUENCY, Hz
FIGURE A-4. - Quarry shot, Type II airblast initial arrival, Type I airblast when reflected
(shot 105/7); coal mine shot, parting, Type I airblast (shot 126/7); and metal
mine shot, Type II airblast (shot 147/7).
40
Shot 126/7 (fig. A-4).--This is a coal mine "parting" shot in a thin (6-
ft) layer of limestone. The peak in the spectra is at 20 Hz. A lack of con-
finement caused the generation of considerable energy in the 20-to 50-Hz
range. The home responded vigorously.
Shot 163/1 (fig. A-5).--A partial misfire with uncovered detonating cord
is illustrated on this large iron mine shot monitoring at about 700 ft. A lot
of high-frequency energy was generated by the detonating cord. The gage,
located in the near field, caused the source to appear to move rather than to
act as a single point.
C5/12
-----
0
TIME, sec
0.5
0 0.5
TIME, sec
(D 60 60 .----r---.--.--~--,
w w
.
"C
50 Shot C5/12 50 Shot 163/1
> 0 40 40
1- :::> 30 30
<t 1- 20 20,..
_J
w _J 10 10
c:: 0..
::!!
<t 0 20 40 60 80 100 0 20 40 60 80 100
FREQUENCY, Hz FREQUENCY, Hz
FIGURE A-5. • Coal mine shot, airblast from a blowout (shot CS/12), and metal mine shot,
airblast from a partial misfire, exposed detonating cord (shot 163/l).
41
TABLE C-1. - Precision sound level meters tested by the Bureau of Mines
1
Dallas Instruments, Inc. Phillip R. Berger VME-Nitro Consult, Vibra-Tech Engineers,
and Associates, Inc., Evanston, Ill. Inc., Hazelton, Pa.
Bradfordwood~ Pa.
Model • •...••.....•••...• St-4 (Vi-Sel Monitors, Safeguard Seismic Model F sound vel- Vibra-tape 1,000 and
Inc., Dallas, Tex.; Unit II. ocity recorder. 2000 series.
EverLert Vibra-Tape
(Vibra-Tech); White Seismo
Sentinel (White Engi-
neering Inc., Joplin, Mo.).
Microphone type ••••••••• 1-1/8-in. ceramic ••••••••••• l-in. ceramic ••••••• l-in. ceramic ••••••• 1-1/8-in. ceramic.
Output method ••••••••.•• Records FM analog on mag- Light beams on Light beams on Records FM analog on
etic tape; separate play direct-write photo- direct-write photo- magnetic tape; anal-
back system for recorded graphic paper. graphic paper. ysis of playback
digital level and analog available from
waveform; analysis avail- Vi bra-Tech.
able from distributors.
Frequency response, Hz •• 5-200 on analog waveform, 3-1/2-200 2-2,000 5-5,000 on 1000 series,
±3 dB nominal. 5-500 on digital. 4-1,000 on 2000 series.
Maximum dynamic dB •• I 137 on tape, 140 on digital 128-148 on paper 140 137 on 1000 series,
range. readout. tape, switchable. 137 or 147, switchable
on 2000 series.
Power source •••••••••••• IRechargeable 12-volt Rechargeable 12- Rechargeable 12- 3- to 6-volt lantern
battery. volt battery. volt battery. battery (1000 series).
2- to 6-volt lantern
battery (2000 series).
Weight ......... kg (lb) .. ll3.6 (30) 12.3 (27) 18.1 (40) 11.6 (26), 1000 series,
12.3 (27), 2000 series.
Dimensions, em (in.):
Length •••••••••••••••• l 52.1 (20.5) 45.8 (18) 49.2 (19.4) 38.1 (15), 1000
43.2 (17), 2000.
Width ••••••••••••••••• 25.4 (10) 35.6 (14) 24.8 (9.8) 33.0 (13)
34.9 (7.3).
Height ................ 117.8 (7) 15.3 (6) 22.9 (9) 19.0 (7.5)
18.4 (7 .3).
Notes ••••••••••••••••••• IOperates up to 1 month Self-contained unit Self-contained unit Other dynamic ranges
unattended; in a standby in aluminum fin- in carry case. optional; electro-
mode, records 4-channel ished briefcase. magnetically shielded
event when vabration case.
exceeds a preset threshold.
1Multiple distributers, see model.
45
"Random" incidence microphones are for use in a diffuse field; that is,
one made up of many reflected waves from all directions that combine to form a
uniform energy-density level. This feature makes such microphones suitable
for indoor use or in other areas with many reflections. At frequencies below
1 kHz, its response is the same as a grazing or perpendicular incidence micro-
phones. "Grazing" and "perpendicular" incidence re.fer to the preferred angle
at which the pressure wave strikes the diaphragm, 90 degrees and 0 degrees,
respectively. The angle is the orientation needed to obtain the best
response. Microphones may also be said to have "free field" response, which
means all sound of interest arrives from one direction with no reflections
such as those found in an enclosed space. Grazing incidence response is also
called pressure response. Any of these three microphones (condenser, elec-
tret, and ceramic) is appropriate since their directional sensitivity is
indistinguishable at airblast frequencies (1, 20, 23).
48
FM tape
recorder
... Channels 5, 6, 7
' I 26 dB amp! ifier
1;3 octave
multifi Iter --
Dual Hr/LO
fi Iter
'
rms
detector
\ \ I
-
Amplifiers
-c -cc
c
·-C'l
1/)
-cc ·-C'l
1/)
"'C C'l
Q)
·- "'C
,_
Q)
-
1/)
,_
"'0
0 Q)
-tJ...
1/)
(.)
Q)
0::
E
,_ ·-
\~ 'I \I
Oscillograph
From the tape recorder, they were first fed into a General Radio Type 1925
Multifilter, which is a spectrum shaper and equalizer and which has ten 1/3-
octave-band, six-pole, active Butterworth filters. These filters range in
center frequency from 3.15 Hz to 2.5 kHz. There is a set of calibrated 1-
dB/step attenuators, one for each of the 30 channels can be output separately
or summed, and internal filters are also available to obtain A-, B-, and C-
weighting for airblast noise analysis (1)·
For the required application, two modifications were made to the filter.
A special low-frequency band was added with a center frequency of 1.6 Hz.
This modification lowered the upper limit of the frequency range to 1.25 kHz.
Then, the filter that was in channels 5, 6, and 7 was replaced by a 26-dB gain
amplifier (fig. F-3). Cables were run from this printed circuit board card to
the housing to allow the introduction of an external filter. This filter
could then be adjusted to a frequency range not available on the Multifilter
itself, or to bypass the 1/3-octave filtering characteristics of the Multi-
filter. This externally filtered signal could then be accessed by using the
channels available on the dummy card. An externally filtered version of the
input signal could then be introduced without providing a separate interface
to the rest of the system. The 26-dB gain was necessary because that gain is
present in the other 1/3-octave-band filters.
The external filter was Rockland 1022F Dual Hi/Lo filter consisting of
two identical, independent filters mounted in the same case, with separate
input and output terminals. This can be set to act as either a high-or a low-
pass filter, with either RC or 4th-order (24-dB/octave) Butterworth character-
istics. The cutoff frequency was digitally selected by a dial on the front of
the instrument, and the dynamic range was 0.1 Hz to 111 kHz. The filter was
used in a band pass configuration accomplished by setting the input in the
high-pass mode and cascading it with the second in the low-pass mode, and then
selecting the frequency range of interest; the 4th-order Butterworth charac-
teristics were used on both. The bandpass-conditioned signal from the Rock-
land was fed into the Multifilter, and the signal was available on its
channels 5-7.
10 KU
470 ,Q
21167
Signal
input
o~----jf---1~--.---i
180 fLf
Full-scale value
0 2
TIME, sec
The GR 1926 rms detector was then directly interfaced to the GR 1925 Mul-
tifilter. The detector measured the rms value of each band of the Multifilter
selected. Any range of bands can be scanned, and the rms value of each
computed (..!:.2_).
The GR 1926 rms detector has a 70-dB dynamic input range and a 60-dB
dynamic output range. The input signals from the multifilter are sampled with
integration times of 1/8, 1/4, 1/2, 1, 2, 4, 8, 16, or 32 sec, depending on
the nature of the signal being processed. The number of samples and sampling
rate depend on the integration time chosen, as shown in table F-1. For most
frequencies the sampling rate was below the Nyquist rate. Since reconstruc-
tion of the input signal was not required, this is of no consequence. The
measurements of the rms energy of each band can be made accurately at a low
sampling rate.
80-pct confidence
Integration Number of Average sampling Average sample limits for indepen-
time, sec samples rate, samples/sec spacing, msec dent samples
(noise input, ±dB)
1/8 128 1,024 0.781 o.s
1/4 256 1,024 .813 .34
1/2 512 1, 024 .877 .24
1 1, 024 1,024 1.00 .17
2 1, 024 512 2.01 .17
4 1, 024 256 4.02 .17
8 1,024 128 8.04 .17
16 1, 024 64 16.08 .17
32 1,024 32 32.2 .17
The GR 1926 rms detector has both analog and digital outputs, and can be
interfaced to a PDP 11 computer, storage oscilloscope, printer, or X-Y
plotter. The output was fed into a Bell & Howell 5-135 oscillograph.
found by adding the floor level; that is, the maximum band level minus 60 dB,
which could be done for each integration period. For our purposes, however,
only the peak energy level was of interest; it alone was measured.
:--
'
T
60 dB
'
22.1 dB
w
I"'
I
0 5
p-r---
~- ---
--
TIME, msec
~
10