Water Front Active
Water Front Active
Abstract
Waterfront retaining walls supporting dry backfill are subjected to hydrostatic pressure on upstream face and earth pressure on the
downstream face. Under seismic conditions, if such a wall retains a submerged backfill, additional hydrodynamic pressures are
generated. This paper pertains to a study in which the effect of earthquakes along with the hydrodynamic pressure including inertial
forces on such a retaining wall is observed. The hydrodynamic pressure is calculated using Westergaard’s approach, while the earth
pressure is calculated using Mononobe-Okabe’s pseudo-static analysis. It is observed that when the horizontal seismic acceleration
coefficient is increased from 0 to 0.2, there is a 57% decrease in the factor of safety of the retaining wall in sliding mode. For investigating
the effect of different parameters, a parametric study is also done. It is observed that if f is increased from 301 to 351, there is an increase
in the factor of safety in the sliding mode by 20.4%. Similar observations were made for other parameters as well. Comparison of results
obtained from the present approach with [Ebeling, R.M., Morrison Jr, E.E., 1992. The seismic design of waterfront retaining structures.
US Army Technical Report ITL-92-11. Washington DC] reveal that the factor of safety for static condition (kh ¼ 0), calculated by both
the approaches, is 1.60 while for an earthquake with kh ¼ 0.2, they differ by 22.5% due to the consideration of wall inertia in the present
study.
r 2007 Elsevier Ltd. All rights reserved.
Keywords: Hydrodynamic pressure; Seismic active earth pressure; Design; Wall inertia; Sliding; Overturning; Factor of safety; Soil and wall friction angle
0029-8018/$ - see front matter r 2007 Elsevier Ltd. All rights reserved.
doi:10.1016/j.oceaneng.2007.03.005
ARTICLE IN PRESS
1948 D. Choudhury, S.M. Ahmad / Ocean Engineering 34 (2007) 1947–1954
However, a very few literature proposed the analysis Steps for the analysis of the rigid retaining wall by
of waterfront retaining wall under the combined action of considering the hydrodynamic pressure generated due to
forces due to water and seismic earth pressure, as most of the submerged backfill along with the seismic active earth
the literature deals with the individual forces acting on the pressures were given only by Ebeling and Morrison (1992).
waterfront retaining wall. For example, the effect of wave However, one of the important aspect of considering the
action on caisson, vertical and sloping walls and other wall inertia, the effect of which on the stability of a
coastal structures had been studied by Kirkgoz and Mengi retaining wall has already been well established, as is
(1987) and by Kirkgoz (1990, 1991 and 1995). Muller and reported by Richards and Elms (1979), Choudhury and
Whittaker (1993) investigated the effect of wave impact on Nimbalkar (2007) and Nimbalkar and Choudhury (2007) is
the sloping walls, while a comparative study for the not addressed properly in the above-mentioned analysis.
evaluation of the design wave impact pressure is again Hence, till today, the complete solution for the combined
reported by Muller and Whittaker (1996). Experimental effect of seismic active earth pressure and hydrodynamic
studies to assess the behaviour of the vertical wall were pressure on the waterfront retaining wall with the
reported by Ramsden (1996) with the details of the consideration of wall inertia is scarce.
development of an empirical expression for calculating The present method completely describes the behaviour
the forces and moments on a vertical wall due to long of a waterfront retaining wall from the stability considera-
waves, bores and surges. For the studies related to the tion in terms of the sliding and overturning modes of
hydrodynamic pressure, Chakrabarti et al. (1978) had failure under earthquake condition. This study is extremely
shown its effect on cellular type cofferdams. New method essential for the design purpose of the waterfront retaining
of analysis for the quay wall including the effect of wall under seismic condition. A generalized case of a
hydrodynamic pressure was described by Nozu et al. waterfront retaining wall, supporting a submerged backfill
(2004). Again, the seismic active earth pressures acting on on one side and water on the other side, under seismic
the rigid retaining wall for dry soil were computed by using conditions including seismic inertial forces is considered.
different methods of analyses like the limit equilibrium
method (Seed and Whitman, 1970; Richards and Elms, 2. Method of analysis
1979; Choudhury and Singh, 2006; Choudhury and
Nimbalkar, 2006, 2007; Nimbalkar and Choudhury, A typical waterfront retaining wall with vertical face
2007), approximate elastic solutions (Matsuo and Ohara, (i.e., y ¼ 01), width ‘b’ and height ‘H’ is shown in Fig. 1. It
1960), two-dimensional wave propagation theory or shear- retains backfill to its full height on one side, referred to as
beam model (Scott, 1973; Veletsos and Younan, 1994; Wu the ‘downstream side’, and water to a height of ‘h’ on the
and Finn, 1999), finite element techniques (Nadim and other side, called as the ‘upstream side’ of the wall. The
Whitman, 1983; Gazetas et al., 2004), numerical simulation ground surface of the backfill is assumed to be horizontal
by using geotechnical software FLAC (Green et al., 2003). (i.e., b ¼ 01) and is submerged to the same level (i.e., ‘h’) up
But none of the above solutions considered the effect of to which the water is standing on the upstream side of the
hydrodynamic pressure. retaining wall. A free body diagram of the wall showing
ARTICLE IN PRESS
D. Choudhury, S.M. Ahmad / Ocean Engineering 34 (2007) 1947–1954 1949
b gsat kh
c ¼ tan1 , (3)
ḡð1 kv Þ
2 2 !
h h
ḡ ¼ gsat þ 1 gd . (4)
Gravity Wall
Water Partially submerged
H H
backfill soil H
h Pae h It is to be noted that the pore pressure ratio ‘ru’, which is
Pw Pw defined as the ratio of excess pore pressure to the initial
vertical stress, incorporated in Eq. (1) above is a simplified
way (as per Ebeling and Morrison, 1992) of simulating the
Fig. 1. A typical gravity type waterfront retaining wall. effect of the excess pore pressure generated due to cyclic
shaking of the soil during an earthquake.
where
7
Pdyn ¼ 12 k h g w h2 . (8)
cos2 ðf y cÞ
K ae ¼ pffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi2 , (2)
cos c cos2 y cosðd þ y þ cÞ 1 þ sinðd þ fÞ sinðf b cÞ= cosðd þ y þ cÞ cosðb yÞ
ARTICLE IN PRESS
1950 D. Choudhury, S.M. Ahmad / Ocean Engineering 34 (2007) 1947–1954
It acts at a height of 0.4h from the base of the wall. On are then given as
the upstream side, this hydrodynamic force acts in a Fr Pstat þ m½ð1 kv ÞW þ Pae sin d
direction opposite to the direction of the hydrostatic force FSslidingr ¼ ¼ 0 (12)
F d r Pstat þ Pdyn þ Pae cos d þ kh W
(Ebeling and Morrison, 1992), while on the downstream
side the direction of both the hydrostatic and hydrody- and
namic forces would be towards the wall, thus creating a
Fr Pstat þ m½ð1 kv ÞW þ Pae sin d
worst possible combination with respect to both the sliding FSslidingf ¼ ¼ 0
F d f Pstat þ 2Pdyn þ Pae cos d þ kh W
and overturning modes of failure of the wall. Though
Matsuo and Ohara (1965) had suggested the hydrodynamic (13)
pressure on the downstream side to be around 70% of that where
on the upstream side, but to consider the worst possible
combination of forces for the design of the wall, similar to m ¼ coefficient of base friction ¼ tan f, (14)
the consideration of Ebeling and Morrison (1992), here in
the present study, the same amount of the hydrodynamic W ¼ weight of the wall ¼ bHgc . (15)
pressure is considered both on the downstream and For the generalized design purpose, Eqs. (12) and (13)
upstream side. can be rewritten in the non-dimensional form as follows:
1 2
2gw ðh=HÞ þ m ð1 k v Þðb=HÞgc þ 12K ae ḡ sin d
FSslidingr ¼ 1 2 7 2 1
,
3. Stability of the wall 2gwe ðh=HÞ þ 12kh gw ðh=HÞ þ 2K ae ḡ cos d þ kh ðb=HÞgc
(16)
Under the action of the above-mentioned forces, the
stability of the wall is checked for both the sliding and 1 2 1
2gw ðh=HÞ þ m ð1 k v Þðb=HÞgc þ 2K ae ḡ sin d
overturning modes of failure using limit equilibrium FSslidingf ¼ 1 2 7 2 1
.
2gwe ðh=HÞ þ 6kh gw ðh=HÞ þ 2K ae ḡ cos d þ kh ðb=HÞgc
method. Depending on the hydraulic conductivity (k) of
(17)
the soil, two different cases viz., restrained water case
(k103 cm/sec) and free water case (kvery high) may
arise for the generation of the hydrodynamic pressure in 3.2. Factor of safety against overturning mode of failure
the backfill soil (Kramer, 1996). For the restrained water
case, the movement of water is assumed to be with the Similarly, by assuming that the seismic active earth
movement of the backfill soil particles and thus it is pressure (Pae) acts at y ¼ 0.5H above the base of the wall
assumed that the hydrodynamic pressure is not present. (Ebeling and Morrison, 1992), the factor of safety against
However, for the free water case, the water is having the overturning mode of failure for both the restrained and
enough space to move freely within the soil, hence, the free water cases, respectively, are given as
additional hydrodynamic pressure is considered. Expres- 1
6gw ðh=HÞ
3
þ 12ðb=HÞ2 ð1 kv Þgc þ 12K ae ḡðb=HÞ sin d
FSoverturningr ¼ 1 .
sions for finding out the factor of safety against the sliding 6gwe ðh=HÞ
3
þ ð2:8=12Þkh gw ðh=HÞ3 þ 14K ae ḡ cos d þ 12kh ðb=HÞgc
and overturning modes of failure are detailed in the (18)
following section.
and
1
gw ðh=HÞ3 þ 12ðb=HÞ2 ð1 kv Þgc þ 12K ae ḡðb=HÞ sin d
3.1. Factor of safety against sliding mode of failure FSoverturningf ¼ 1 6 3 5:6 3 1 1
.
6gwe ðh=HÞ þ 12 kh gw ðh=HÞ þ 4K ae ḡ cos d þ 2k h ðb=HÞgc
Table 1 2.5
Values/range of different parameters chosen for the present study b/H = 0.4; φ = 30° ; δ = φ/2; kv= kh/2; ru= 0.2
FSoverturning
1.5 h/H = 0.8 (restrained)
b/H 0.4 h/H = 0.4 (free)
h/H 0, 0.4, 0.8 h/H = 0.8 (free)
kh 0, 0.1, 0.2, 0.3, 0.4 1.0
kv 0, kh/2, kh
ru 0.2 0.5
gc, gsat, gd, gw 25, 19, 16 and 10 kN/m3 respectively
f (degree) 25, 30, 35, 40
d (degree) f/2, 0, f/2 0.0
0.0 0.1 0.2 0.3 0.4
Horizontal seismic acceleration coefficient, kh
FSsliding
2.0 φ = 35° (free)
1.5
φ = 30° (free)
1.5
1.0 φ = 25° (free)
1.0
0.5
0.5
0.0
0.0 0.1 0.2 0.3 0.4 0.0
Horizonal seismic acceleration coefficient, kh 0.0 0.1 0.2 0.3 0.4
Horizontal seismic acceleration coefficient, kh
Fig. 3. Factor of safety in sliding mode for different h/H values.
Fig. 5. Effect of f on sliding stability.
φ = 25° (restrained)
considered in the present analysis are given in Table 1. 1.5
φ = 35° (free)
Effect of the various parameters on the sliding and φ = 30° (free)
overturning stability of the wall with respect to the value 1.0 φ = 25° (free)
of water to wall height ratio (h/H), soil friction angle (f),
wall friction angle (d), and the coefficients of horizontal 0.5
and vertical seismic accelerations (kh and kv) are discussed
0.0
in Figs. 3–10. 0.0 0.1 0.2 0.3 0.4
Horizontal seismic acceleration coefficient, kh
4.1. Effect of the horizontal seismic acceleration coefficient
(kh) Fig. 6. Effect of f on overturning stability.
2.5 3.0
b/H = 0.4; h/H = 0.8; φ = 30°; kv= kh/2; ru= 0.2 b/H = 0.4; h/H = 0.8; φ = 30°; δ = φ/2; ru= 0.2
2.0 2.5 kv= 0.0 (restrained)
δ = -φ/2 (restrained)
δ = 0.0° (restrained) kv= kh/2 (restrained)
2.0
FSoverturning
δ = φ/2 (restrained) kv= kh (restrained)
1.5
FSsliding
0.0 0.0
0.0 0.1 0.2 0.3 0.4 0.0 0.1 0.2 0.3 0.4
Horizontal seismic acceleration coefficient, kh Horizontal seismic accleration coefficient, kh
2.5 the value of soil friction angle f is nearly constant for all
b/H=0.4; h/H = 0.8; φ = 30°; kv= kh/2; ru= 0.2 values of kh and is true for the overturning case also
2.0 δ = -φ/2 (restrained) (Fig. 6). Also, the trend is similar both for the free and
δ = 0.0° (restrained) restrained water cases, except for the fact that the value for
δ = φ/2 (restrained)
FSoverturning
1.5 δ = -φ/2 (free) free water case is slightly lower than the value of restrained
δ = 0.0° (free) water case. Another important observation from these
δ = φ/2 (free)
1.0 figures is that with an increase in f, the shear fluidization
phenomenon can be avoided.
0.5
Fig. 9. Effect of kv on sliding stability. As shown in Fig. 9, with the increase in the vertical
seismic acceleration coefficient, kv from 0 to kh, the factor
the stable wall under static condition has failed in both the of safety against sliding mode reduces (for kh ¼ 0.1,
sliding and overturning modes (FSo1 in Figs. 3 and 4). b/H ¼ 0.4, h/H ¼ 0.8, f ¼ 301 and ru ¼ 0.2) by about
4%, which may be considered as marginal. Overturning
4.2. Effect of soil friction angle (f) mode of failure of the wall shows the similar behaviour as
can be seen from Fig. 10.
Figs. 5 and 6 respectively show the variation of factor of
safety in the sliding and overturning modes of failure for 5. Comparison of results
different f values. With the increase in the value of f from
301 to 351, there is 20.4% increase in the factor of safety For the purpose of verifying the present methodology for
against the sliding mode of failure (Fig. 5) for kh ¼ 0.1, design, the results obtained must be compared with existing
b/H ¼ 0.4, h/H ¼ 0.8, d ¼ f/2, kv ¼ kh/2 and ru ¼ 0.2. The works. However, as already mentioned, for the waterfront
rate of decrease in factor of safety value with decrease in retaining wall subjected to combined hydrodynamic
ARTICLE IN PRESS
D. Choudhury, S.M. Ahmad / Ocean Engineering 34 (2007) 1947–1954 1953
1.0
6. Conclusions
0.5
The study shows the importance to develop a separate
0.0 design methodology for a waterfront retaining wall under
0.0 0.1 0.2 0.3 0.4 earthquake condition. The stability of the wall decreases
Horizontal seismic acceleration coefficient, kh significantly during an earthquake. An easy methodology
to design the section of the waterfront retaining wall
Fig. 11. Comparison between present analysis and the one adopted by subjected to the combined action of hydrodynamic
Ebeling and Morrison (1992) for sliding stability.
pressure and seismic active earth pressure is described
through the closed-form solutions to obtain the factor of
2.0 safety against sliding and overturning modes of failure.
b/H = 0.4; h/H=0.8; φ = 30°; δ = φ/2; kv= kh/2; ru= 0.2
From the typical results it is observed that for a given wall
Ebeling and Morrison (1992)
1.5 Present
section and other soil and water parameters remaining
constant, the factor of safety in overturning mode is less
FSoverturning
Acknowledgement
pressure and seismic active earth pressure, the only work
The authors gratefully acknowledge the critical reviews
which can found out is the one by Ebeling and Morrison
and helpful suggestions made by the anonymous reviewers.
(1992). Figs. 11 and 12 present a comparison between the
results of the present study and the one obtained by the
approach used by Ebeling and Morrison (1992). A keen References
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