waterfront sheet pile walls si:xejected to e …
TRANSCRIPT
CUIMR-Q � 90 � 00l C3LOAN COPY QHLY
WATERFRONT SHEET PILE WALLS SI:XeJECTED TOE 4&THQUABK SK&HNG: ANALYSIS METHOD
Final Beycet on Sea Grant eject 8/OK-8Submitted to Sea Grant Pmgram
Priacipa1 Investigator:
Toycehi Nogmai
8 'W ~l I A~ybyUniversi,ty of Camfornia at SanDieg~ La JoHa, CA 92t;83
TABLE OF COM.'%20 S
1. INTRODUCTION
1.1 Pevious Studies Related to Seismic Earth Pressure onRetaining walls
1.2 Observation of Earthquake Damages ofWaterfront Sheet Pile Walls
1.3 Objective of Study
2. FINITE ELEMENT FORMULATION.
2.1 Soil Elements.
2.2 Joint Elements at Soil-Wall Interface....
3. TIME INTEGRATION FOR SOLVING EQUATION.....
4. VERIFICATIONS
5. EXAMPLE OF COMPUTED BEHAVIOR OF WATERFRONTSHEET PILE SUBJECTED TO EARTHQUAKE SM&XlVG........
REFERENCES
L. IKIRODUCTIGN
L.l Previous Studies Related to Seismic Earth Pres~~xm~ on Retaining%alls
Seismic effects on rigid retaining walls i.e. gravity walls! have been
studied both theoretically and experimentally. Mononobe �919! and Okabe
�926! proposed a simplified formulation to evaluate the seismic lateral
earth pressure on a retaining wall backfilled with dry cohesionless
naturals Mononobe-Okabe method!. Their method is based on a plastic
limit condition and assumes a triangular distribution of earth pressure
along the waU height. According to this pressure distribution, the total
force is acting at the one-third of the wall height from the bottom. Using
small scale rigid wall models with dry sand backfill, the earth pressure due
to dynamic ground. shaking was investigated experimentaHy by using a
shake table Mononobe and Matsuo, 1919; Jacobsen, 1939; Matsuo, 1941; and
Ishii, Arai and Tsuchida, 1960!. The experimental results showed that the
maximum lateral earth pressure was roughly equal to that predicted by the
Mononobe-Okabe, but the location of the total lateral force was higher than
one-third of the wall height. It was also shown that the increase of the
permanent lateral earth pressure aRer the shaking was substantially
higher than the maximum dynamic transient pressure during shaking.
Prakash and Basavanna �969! and Seed and Whitman �970! modified the
Mononobe-Okabe method and assumed a more realistic distribution of
earthquake lateral pressure. Sabzevari and. Ghahramani �974! used the
incremental rigid plasticity theory to obtain analytical expressions and
construct stress displacement and velocity Belds behind the wall. This
method enables us to compute the lateral earth pressure for various types ofrigid wall displacement.
Formulations based on elastic analysis were also developed for theevaluation of the dynamic lateral earth pressure. Matsuo and Ohara �965}and Tajimi �973! solved elastic wave equations to obtain the formulations.Scott �973! modeled the soil and wall system as an elastic vertical shearbeam and a rigid wall connected each other by distributed horizontalWinkler springs and developed the formulae to compute the dynamic earthpressure. Given earthquake excitation at the base of the beam, the beamsimulates the free-6eld earthquake ground motion, and Kinkier springsproduce the soil-wall interaction force i.e. lateral earth pressure!. Thoseformulations based on elastic analysis generally estimate the maximumlateral earth pressure significantly higher than those estimated by theformulations based on a plastic limit condition. Elastic analysis may bejusti6ed if the lateral response of the waH is not large enough to produce aplastic limit condition behind the wall.
Lt depends on the displacement of the wall whether the backfiH soil isin an elastic condition or plastic limit condition. The nonlinear Rnite
element method is a convenient analysis tool to evaluate the lateral earthpressure since the conditions in the soil are automatically adjustedaccording to the magnitude of strains developed in the soil. Potts andPourier �986! used a Gnite element method and. found that the
displacement pattern of the wall highly afFects the amount of the waHdisplacement required to fully mobilize the plastic limit condition behindthe waH and. the pressure distribution. Those indicate that the wall
Qexibility aFects the lateral earth pi'essure on the waH. Kuralowicz and
Tejchman ].984! investigated experimentally the static earth pressure on
rigid and. flexible sheet-pile walls in cohesionless soil. It was observed that
the distribution shape of the lateral earth pressure on a flexible wall was
nonlinear, although that on a, rigid wall was nearly triangular. Ayala,
Rorno and Goinez �985! investigated the maximum bending moment of
flexible walls induced by seismic earth pressure by using the Rnite element
method. Flexibility of the waH was found to afYect the maximum moment.
Kurata, Arai and Yokoi �965! conducted shaking table tests with a
small scale anchored sheet-pile wall model in dry cohesionless soil. They
observed that the ground shaking increased the lateral earth pressure
substantially in the vicinity of the anchor level but did. not increase much in
the middle part of the waH. This is due to redistribution of the lateral earth
pressure resulting from Qexural deformation of the wall. The total lateral
earth pressure observed during shaking was smaller than that computed
by the Mononobe-Okabe method. It wa.s also observed that the increase of
permanent 1ateral earth pressure due to the permanent soil deformation
was much larger than the transient dynamic earth pressure. Murphy
�960! also conducted model tests on an anchored sheet-pile wall subjected
to earthquake shaking. It was pointed out that the wall translated outward
without tilting until the anchor puH failed. As essentially planar slip
surface was observed in the backfiH soil. Simitar planer slip surface was
observed by Bolton and Steehnan �985!.
When the backGD soil is submerged, a portion of the water in the
pores of the soil mass moves with the lateral soil skeleton restrained water!
and the other portion moves freely during ground shaking free water!.
The hydrodynamic pressure in the bacldill against the wall is due to the
motion of the free water, and this depends on the volume of the free water.
Anzo �936! formulated the hydrodynamic pressure in the submerged
backfi11 against the wall. The formulation was based on a rigid soil
skeleton, Darcy's flow and Navier-Stokes equations. According to this
formulation, the hydrodynamic pressure in the soil never exceeds the value
computed by Westergard's formula and is smaller for a lower permeability.
iVIatsuo and Ohara j.965! conducted model tests on the wall with
submerged backfill sand. The observed hydrodynamic pressure was
somewhat larger than that computed by Westergard's formula.
Liquefaction was observed in some of those tests. Ishibashi, Matsuzawa
and Kawamura �985! proposed the method estimate the dynamic pressure
against the wall retaining submerged. backs soil. The method adopts the
Mononobe-Okabe method with the soil weight increased by the restrained
water weight! for earth pressure and simplified Anzo's formula for
hydrodynamic pressure.
Towhata and Islam �987! viewed that the magnitude of permanent
wall displacement was the most critical phenomena for the judgement of
the degree of seismic damage of anchored bulkheads. Based on this view,they developed a simple method to compute the lateral movement of
anchored bulkheads induced by earthquake shaking assuming a
triangular sliding wedge behind the wall. They considered that the e8ect of
liquefaction in backfill was particularly important and thus was taken into
account in the method.
12 Ok~ation of Earthquake Damages to Waterfront Sheet Pile Walls
The Niigata earthquake in 1964 caused substantial damages toretaining structures. Most of those damages were closely connected to the
development of excess pore water pressure associated with liquefactionprocess.
The ministry of Transportation �964! published a detailed report on
earthquake damages in Niigata harbor facilities. The report indicates that
substantial translation of walls occurred toward the mater at the mall next
to Yamanoshota Wharf, due to loose reclaimed backfiHs. The North and
South Wharfs were sufFered from excessive two-meter movement of their
walls. Similar movement was detected in the Bandai-Jima area as well.
The North bank of the Shinano River completely collapsed, accompanied byoverall displacement of backfill toward the river. Although the reportconcluded. that most sheet-pile wall damages were due to tilting, it alsomentioned that lateral translation took place in walls of shallow
embedment. At the areas of al1 those anchored bulkheads, evidences of
liquefaction mere reported.
13 Objective of the Study
The objective of the project is to develop an analysis tool for computingthe behavior and conditions of waterfront sheet pile walls during and rightafter the earthquake ground shaking. Key factors for the judgement of theseismic performance of waterfront anchor bulkheads are bending momentin the mall and permanent lateral movement of waH, induced by
earthquake shaking. According to the previous section, those are affected
mainly by elastic and inelastic soil behavior, excess porewater pressure,
flexibility of wall, motions of backfill and wall, and hdro-dynamic pressure
at both front and back sides of the wall. The finite element method may be
the most convenient analysis method to consider rationally all of those
important factors affecting the performance of walls, and thus was
developed in the project.
Fig. 1.1 shows finite element models of a waterfront sheet pile waH.
The effect of water at the front side of the wall is taken into account by added
masses attached at the nodes located at the water-wall and water-soil
interfaces. Those masses are active for motions only in the component
normal to the interface. Soil elements are formulated treating the soil
mass as a water-saturated two phase mixture. This enables soil elements
to simulate the coupling between porewater motions and soil frame
motions, generation and dissipation of excess porewater pressure in a soil
mass, and effects of excess porewater pressure on the soil frame behavior.
Discontinuity of displacements develops at the soil-wall interface due to
large difFerence in the stiffnesses between those of the waH and soil and due
to sliding and separation between the waQ and soil. This requires special
e1ements, termed joint elements, to accomodate such behaviors at the
interface.
I. FIMIIR RIRMENT FORt IULITION
2.1 Soil Elements
Submerged soil is treated. as a Quid-saturated porous medium. The
nonlinear behavior is implemented in the stress-strain relationship of thesoil frame.
�! De6nitions of Valuables
Porosity n is defined as
Vn�
V + V, �.1!
where Vf = volume or pores or fluid; and. Vs = volume of solid.
Relation given in Eq. 1 can be transformed to density relationship as
p = � � n!p, + iipf �.2!
7
where p, ps and pt= mass densities of solid-Quid mixture, solid and fiuid,
respectively. ln order to describe the deformation of a mixture,
deformations of the two phases are identifled separately. The componentsof deformation of the so1id can be denoted. by u; i = 1, 2, 3! and componentsof displacement of the Quid. can be denoted by U; i = 1, 2, 3!. i denotes
coordinate axes. The amount of Quid displaced from the solid skeleton, Q;,is obtained as
Q. = A,u U, - u,! �-3!
where A; = area of mixture n.ormal to the ith direction.
face of the mixture is obtained as
%, = � = u U. - u.! �-4!
The strains in the solid skeleton are dered as
�.5a!
or
<e> � D.j r�.5b!
where
={ ll 22 33 21 23 31}
0 oBx! 3Q8
ax,
0 0 0Bx
0
a a
B.] =
The displacement of fluid relative to solid skeleton, averaged over the
� 9!
Strains in the solid grains induced by pore pressure can be expressed byusing the bulk modulus for solid as
�,10!
Deformation of solid skeleton caused by the effective stress a;J' is related to cfJ!< through the constitutive terms or D1JQ1
�.1 j.!
Combining Eqs. 7 through ll, the foUowing relations are obtained:
PijkI kj 3K ijkl kl P ij �.12!
which is rearranged as
a,. = 0,.�, e�, + ap5., �.13!
where
10
Similarly, strains are also decomposed into two parts. Part of the strain iscaused by deformation of grains due to pore pressure, and the part iscaused by deformation of grains and skeleton due to effective stress. Thiscan. be expressed as
�! Amount of fluid flowing out of 2, = change of volume of pores!;
�! Volume change in solid due to p, = p�-n!/K>!;
�! Volume change due to p, = n~!; and
�! volume change of solid. due to effective stress, < = a; /3
Thus, the continuity condition. is formulated as
e., = �-n! + � + 3KP AP ii1E �.15!
Rewriting 4�" in Eq. 2.15 with Eqs. 2.9, 2.10 and 2.11 leads to
1-n
F =Q .p+ � { "ld kl ill P! - Lj 3K,
or
11
Continuity of Quid Qow wi11 be formulated in order to obtain a relation
for pore pressure taking into the volumetric change of each phase. Thetotal volume change of the mixture, e;;, consists of the sum of the followingparts:
P =QC+ aug! �.16!
where
1 n an+-Q Kf K,
Equations for constitutive relation of porous material aresummarized as
�,13!
P =Q E+ aQ�! �.16!
i ' ijkA>9K,
1 n an+��.17!
d<.. = D..q! +q a' dp 5.. �.18!
�.18!
where
12
For nonlinear behavior, the constitutive relation needs to be
expressed in incremental form. The incremental forms of Eqs. 2.13 and2.16 are
ij ijkl kl
9Ks � 20!
ep [de,! + r> dp � 2~!
gp -gt r> dE!+ Jg]
where
1 n 1n� � � +�,23!
and
T da! -f«�«zz <zz «,z zz
T<«k = ~zz ~zz ~zz ~zz ~zz ~zz} �.24!
rk I I I 0 0 0!
�! +ammic Egmlibrimn Kyxation
Two equations are required to describe the equilibrium conditions of
two phase mixture. 'We wiH look at the equilibrium con.ditions in the
13
and D<;>g~ is incremental constitutive tensor for skeleton. The value a~ is
nearly equal to 1 since the second term at the right hand side of Zq. 20 isvery small compared with the erst term Zienkeiewicz at al., 1984!. Zqs.2.18 and 19 with a = 1 can be rewritten in a matrix form as
mixture as a whole and in the fluid phase first.. Masses of a solid phaseand fluid phase in a unit volume of mixture are respectively l-n!ps and
npg. Therefore, the equilibrium conditions in mixture as a whole are
described as
a, + I-n!p,b, + np,b. - � � n!p,ii, - np,U. =0 �.25!
w =n U- u! =k.. h.<J ~ 3 � 26!
where "~ = 3 w U u!/Bt; k;j = component of permeability tensor; h>j =gradient of fluid head in the jth direction. Under the steady state
conditions, the gradient of the head is composed of pressure gradient, bodyforce gradient and inertia of fluid. This is written as
h. =p, + p<b, - pfU, �,27!
Combining Eqs. 2.26 and 2.27, equilibrium conditions in fluid phase can bedescribed as
p . + p<b, = pfU, + k,. n U. - ia,! � 28!
Substitution of AU; in Eq. 2.28 into Eq. 2.25 yields
14
where b; = ith component of body force per unit mass; u = B~u/Bt2; and U =
32U/Bt2. The equilibrium conditions of fluid phase will be developed from thegeneralized Darcy's equation described by
o; + pb, - I-n!p,ii, + k,. n U. - u.! -np, - npfb. = 0 � 29!
Using a;> expressed by Eq. 2.7, Zq. 2.29 results in equilibrium condition in
solid skeleton expressed as
a; + I n!p;+ I n!pub; I n!p ii+k; n U; i.! =0 �.30!
Hereafter, Eqs. 2.30 and 2. 28 will used for two equilibrium equations
for two phase mixture. Those will be rewritten in a matrix form as
T T TfIU a'! + �-n! ~! p+ !-n!p, b! - !-n!p, !!+ n' k! 1 !! � ! = 0 �.3 !
~! p+ pf ] pf U j >I:kl � - u! = �! � 32!
@uk D-l fo'J + I-n! V! p+ Ii-n!p, b! - I-n!p, ii! +n Ik] U-uj dQ=0�.33!
where < = the domain of interest; �ul = components of virtual
displacement compatible with u!. Similarly, application of virtual workprinciple to Eq. 2.32 results in
15
�! Finite Element Formulation for Numerical Evaluation
The principle of virtual work requires that for an arbitrary virtual
displacement, the work done through Eqs. 2.31 and 2.32 over the domain of
interest must be equal to zero. This requirement on. Eq. 2.31 is given by
The domain is divided into finite elements. Within an element, the
variables are approximated in terms of the values of variables at nodal
points such that
u! = [K u! <! = ll:N! U! �.39!
where [+ = matrix of interpolation function. for {u! and U!; <! and U! =
vectors of nodal variables of u! and U!, respectively. Then, since ~ is
function of spatial coordinates only, it is also approximated that
� 40!
Similarly, �u! and. {5U! are approximated by
{5u! =PU{5u!. {5U! = PU{5U! �.41!
Using j de6ned by Eq. 2.6a with w! = n{U-u!, Eq. 2.22 can be
rewritten as
dp = Q r da + dg!= $ r LJ�u + n ~ dU - n V �u !=Q l-n!{V! du! +Qn{7! dU! �.42!
17
Substitution of Eq. 2.42 and Eqs. 2. 39 through Eq. 2.4L into Zqs.2. 35 and 2.36leads to
Avl U! - C,] !+ C,! U! :K2] !+t:K3] ~! = <v! � 44!
where
t'MJ = �- !p, N] N] dQ
Mvl=~pf W N] d~T
C,] =n 'N] I'k] [N] dQ
T
[K,] =�-rl! Q <! [N] �! IN] dQ
[K ] = !-n!nQ|t[V! [N]! V! [N] dQ
T
[K,]=n Q ~! [N] V'! >]aO
f ! = l-n!P, [NJ b! dQ+ [N] t! dI + I-a! {iV] p! dlA r r
fv! = npf [N] �! dQ+ n [N] f!! dI
18
[Mg u! + [C] u! - [C~] !! +f[Bg u! dQ+ [K] [u! + [K ] U! = [ ] Zu3!
Combining Eqs. 2.43 and 2.44, we have
[M] dvj + [Cj dvj + [K] dvj - O] c9.j = dfj
where 0 M�
19
dh
dv! =dU
df� >! =
dfU
Incremental equation of equilibrium can be written as
[M] hdv! + [C] duiv! + [K] kdv! - Pg &! = hdf! �.45!
�! ShessWtxain Constitutive Equation
Elasto-plastic behavior is considered in the stress-strain relationship
It is assumed that the following requirements are met:
of the porous skeleton. In this report four di8erent yieM criteria, the
Trescas, Von Mises, Mohr-Coulomb and Dru.cker-Prager criteria, are
employed. The latter two are applicable to concrete, rocks and soils.
l. An explicit relationship between stress and strain must be
formulated to describe material behavior under elastic conditions,
i.e. before the onset of plastic deformation.
2. A yield criterion indicating the stress level at which plastic flow
comments must be postulated.
3. A relationship between stress and strain must be developed for post
yield behavior, i.e. when the deformation is made up of both elastic
and plastic components.
Before the onset of plastic yielding, the relationship between stress
and strain is given by the standard linear elastic expression.
�.80!ij ijkl kl
where D;>g1 = tensor of elastic constant. For an isotropic material, D;>g1 isexpressed in the form of
D, ki = X5.�.5�! + u.5.�5.! + ph, 5.� �,81!
where A. and p. =Lame's constants; and 51> = Kronecker delta deemed by
1 if i=j5
0 if iwj �.82!
a. Yield Cxiteria
The yield criterion determines the stress level at which plastic
deformation begins. 76th the stress invariants de6ned by
21
�.84}
the yield criterion can be written in the form of
f{J ', J '! = S s! �.85!
where f and S = some functions to be determined experimentally; s =hardening parameter; J2' and J3' = the second and third invariants of the
deviatoric stresses expressed by
G;. = G.. � � 5.. Zkkij ij 3 lj kk {2.86!
Tr a Id ' ri: This states that the yielding begins when themaximum shear stress reaches to a certain value or
a - cr = S s!1 3 �.87!
for ai > a2 > cd ~here cubi, o2, and a3 = principle stresses.
J '! = S s! �.88}
The second deviatoric stress invariant, J2', can. be explicitly written as
22
J =a..l ii
J = � a..o..12 2 1J 1J
J = � cr, a. cr.13 3 ij jk kl
VnM' ' d
reaches to a value
n: This states that yielding occurs when Jg'
�.89!
Yield criteria, Eq. 2.88 may be further written as
5=&3$ s! � 90!
where < is termed effective stress, generalized stress or equivalent stress,
expressed as
<z= J3 J.'! = � {a,.' cr..'! �.91!
This is a generalization of the Coulomb
friction failure law de6ned by
�.93!
where z and cr�= shear and normal stresses, respectively; c = cohesion; and
p = internal friction. angle. For a'y > a'2 > cry, Eq. 2.93 can be rewritten as
�.94!
or rearranging
cr, � o'>! = 2c cos Q- cz,+a>! sin P �.95!
: This is a modi5cation of the Von loses
23
yield criterion for making it dependent on hydrostatic pressure like the
Mohr-Coulomb criteria. The influence of a hydrostatic stress component on.
�.96!
The yield surface defined by Zq. 2.96 in the principal stress space is a
circular cone whereas that defined by the Mohr-Coulomb is a conical yield
surface whose normal section is an irregular hexagon. The followingexpressions for a and S makes the Drucker-Prager circle coincide with the
outer apices of the Mohr-Coulomb hexagon at any section.:
2 siii PC=
l 3 {3 - sin !! �.97!
6c cos 4
l3 �- sin 4! � 98!
Coincidence with the inner apices of the Mohr-Coulomb hexagon isprovided by
2 siii P
P3 � + sin !! �.99!
S 6c coshR3�+ sin 4! �.10G!
W h St
If f = s represents a yield surface, the elastic and plastic
conditions exist respectively when f < s and f = s. At plastic state, the
24
yielding was introduced by inclusion of an additional term in the Von Misesexpression given
incremental change in the yield function due to an incremental stress
change is
�. 105!
Then if:
elastic unloading occurs elastic behavior! and the stress
point returns inside the yield surface.
neutral loading plastic behavior for a perfect plastic
material! and stress point remains on the yield surface.
df>0 plastic loading plastic behavior for a strain hardening
material! and the stress point remains on the expanding
yield surface.
c. Zlasto-P13stic StxmsHtrain Relationship
da,. = da,.!, + de,,!> �.106!
The elastic strain increment is related to the stress increment by Zq. 2.80.
Decomposing the stress terms into their deviatoric and hydrostatic
components, the elastic component of the incremental strain can be
expressed as
25
After initial yielding the material behavior will be partly elastic and
partly plastic. During any increment of stress, the changes of strain are
assumed. to be divisible into elastic and plastic components such that
dq a = H' q! �. 114!
For the u.niaxial case ay = a, az = a3 = 0!, Eq. 2.91 leads to incremental
effective stress and effective strain expressed respectively as
da = � {da..' da..' ! = da3 13 1J �.115!
1
d =g � { de,,'! de,,'! f =defz�.116!
Substitution of E ps. 2.115 and 2.116 into Eq. 2.114 leads to
da da I E T
�.117!de - dec dada da
Adopting the strain hardening hypothesis, Zq. 2. 85 can be rewrittenas
F a, s! = f a! - S s! = 0 �.121!
DifFerentiating Eq. 2.121, we have
dF = da+ � ds =0BF= aa a. �.122!
or
27
where ET = tangent modulus. Thus, the hardening function H' = can. bedetermined experimentally from a simple uniaxial yield test.
�.123!
where
~F BF 3F BF BF BF a! = Ba,' 3 z ' 3a,' 8 'W '&t�y �.124!
A= � � ds1 8F= ~as �-125!
The vector a! is termed the flow vector.
Eq. 2.112 can be rewritten as
T
de! = D] «!+~Ia~7 �.126!
Premultiplying both sides of Zq. 2.126 by a!T D] and. eliminating a!T ds by
use of Eq. 2.123, the plastic multiplier d~ can be expressed as
a! D] de! �.127!A + a! D] a!
epde =D de �.128!
where
28
Substitution of Eq. 2.127 into Eq. 2.126, with dDT = aTD and dD = Da, results
D'=DA+dD a
7 �.129!
work hardening hypothesis, ds is
ds=o de �.130!
Zq. 2.126 can be rewritten for uniaxial condition as
A= 1 dods~ ds �.131!
Employing the normality condition in Eq. 2.130 results in
ds =&a a' � 132!
Eq. 2.124 for uniaxial condition is
da�.133!
Using Euler's theorezn applicable to all homogeneous function of order one,
we have
�.13$
or
a~~= a �.135!
Bf3�
The uniaxial conditions, cry = a and a~ = ag = 0, are considered. With
Substituting Eqs. 2.133 and 2.135 into Eqs. 2.132 and 2.131, ~ and A are
found to be
�.136!
A=H'� 137!
Thus, A is the second slope of the uniaxial stress-strain curve and can be
deternnned experimentally from Eq. 2. 117.
It is written as
sin 38 =-�2
J~'! ~�.»8!
Then, the total principal stresses can be expressed by
�.139!sin 8+~" !
3
The focus yield criteria can now be rewritten in terms of Jy, J g' and 8 asfollows:
Tresca yield criterion1
2{J>'! = a s! �.140!
Von Mises yield criterion
30
I
2 J2'!sin 8+ 2z!
sin 8
1
1J 3
1
bohr-Coulomb yield criterionI
� J sin P+ J '! {cos 8 - � sin 8 sin g! = c cos $1 13 j.
r3�. 142!
Drucker-Prager yield criterion1
aJ, + J '! =S�.143!
where e and S are given in Zqs. 2.97 through 2.100.
In order to calculate the Dep matrix given in Eq. 2.129, it is requiredto express the flow vector a and the elasticity matrix D in a form suitable for
numerical computation. The explicit form of the elasticity matrix D forplane strain condition can be written as
1 N 0 N
N 1 0 N
�.144!0 0 � -NO2v
N N 0 1
where N = v/ l-v!. The flow vector a for plane strain condition can bewritten as
BF BF BF a! = Ba ' Bcz' >
x y xy {2.146!
The specific form of the vector, a!, is given by
31
a! = C, a<! + C2 q! + C3 Q t',2 147!
where
a ! =�,1,0,1!
a ! = ~~ o�', a�', 2x��, a,' !'7 J '
�.148!
~! = +y' +z' + ~ +x' +z' + +z ~xy ~+x' +y' ~xy +
and the deviatoric stress invariants are
1 2r = ' ~ '! + ~ '! + a '! + ~ '2 z xy {2.149!
�.150!
Tresca yield criterion
C =0I
C> = 2 cos 8 � + tan e tan 36! g.151'
lY sineo 3e
Von Mises yield criterion
32
The constants Cl, C2 and C3 are to de6ne the yield surface and are given asfollows:.
22 Joint Element at Soil-WaH Interface
The nodal displacement vector in the s-n local coordinate system is
defined as
�.157!
and also the strain vector as
�.158!
where y, e and m are respectively average difFerential displacements in s
and n directions and angular opening between the two sides, expressed by
U.+U ~ ti.+usj sl si sk
7 2 2u .+U
nj nl6
U -+u ~ni ak �.159!2
Q -U U,. -Unl nk ~niCO�
34
A discontinuity of the displacements develops at the soil-wall
interface due to large difference between the stiffnesses of the wall and soil
and due to sliding and separation between the waO and soil. The joint
element originally developed by Goodman �976! can simulates such soil-
wall interface behaviors. Referring to Fig. 2.1, the joint element is
formulated in the following:
�.160!
where
02
0I
2
0IL
0I2
02
0I2 �.161!
0 - � 0IL
The stress vector in the joint element is dered as
{ a! = c�,, a�, Mo!T
�.162!
where s�s, a�and Mp are respectively shear and normal stresses and
monMnt, expressed by
g= � f +f!Isj sl
a�= � f, + f,! �.163!
The nodal force vector is de6ned as
�.164!
The relationship defined in Zq. 2.159 can be rewritten in the matrix formsuch that
Eqs. 2.I63 and 2.164 with fs; = -f» result in
� 165! fJ =%] o!
where
0 0L2
0 LL
0 02
L I02 L
0 02
0 L I2 L
0 02
0 L I2 L
�.166!
The stress-strain relations at the soil-wall interface are assumed to
be as shown in Fig. 2.2. Yield shear stress w> is assumed. to be
c + G� tan Q s< 0!
0 e >0!�.167!
where c and ~ = cohesion and friction angle at the soil-wall interface,respectively. Furthermore, the following relationship is assumed:
4L k�m a<0!I 3
0 e >0!�.168!
36
at the soil-wall interface is obtained as
T11
d~! = ~f! p�! du'! = ~][C! L ]{du'! �.169!
where
�,170!
with
�.171!
Thus the stiFness matrix of the joint element in local coordinates is
�.172!
with
k, 0 -ks 0
0 2k 0 -2k�
-k, 0 k, 0 �.173!
37
With Zqs. 2.160 and 165, the incremental force-displacement relation
k, 0 -k, 0
0 0 0 0
k, 0 ks 0
0 0 0 0
�.174!
The displacement and force vectors in the local coordinate system are
expressed by those in the global coordinate system as
f~'l = f2 <!
t I = fT]f~] �.175!
where
ft] fo] f0] f0]
fo] «] fO] f0]
f0] f0] f~] fO] �.176!
fo] fO] fo] ft]
with
cos e sin a
�, 177!-sin a cos m
�.178!
Then, the tangential stiffness matrix in the global coordinate system can be
obtained as
3. TIME I%I'EGRATION FOR SOLVING EQUATION
Incremental equation of equilibrium equation for the problemconsidered is written in the form of
[M] {dii! + [C] du J + [Kj {du J = {dff
For the assumed linear variation of the acceleration. and the correspondingquadratic and cubic variations of the velocity and displacement, the Taylorexpansions at the end of the interval ht leads to the following equations for
increments of velocity and displacement:
huf = tijht hQ!2
�.3!
Hence, Eqs. 3.2 and 3.3 result in the incremental displacement and
incremental velocity expressed in terms of incremental displacement asfollows:
� 4!
�.5!
Introducing Wilson 9 method, Eqs. 3.4 and 3.5 result in
39
where
equation of motion:
�.9!
where
CI = KI+ � MI+NCI
ipj = Af! M] ! + 3 uj +[CI
ASolving Eq.3.9 for ~u, the incremental acceleration ~u is
�. 11!
Auj = � Du! - � u! -3 iij j
and. thus
Substituting Eqs. 3.7 and 3.8 into Eq. 3.1 leads to the following
The initial acceleration for next time step is given as
�. 14!
and the entire process may be repeated for any desired number of fime
increments to compute the response time history.
41
4. VRRIFICATIGNS
4.1 Static Pmblems
Young's modulus E! = 6000 psf
Poisson's ratio v! = 0.4
Coef. of permeability k! = 2.5 x 10< ft/day
Density of water ~ g! = 62.5 pcf
The time factor T is de6ned as
C t
H� I!
where c< = coeffxcient of consolidation; t = tizne; and H = height of the soil
column. The coefBcient of consolidation cv for the conditions considered in
this problem is 5.1428 x 10-2 ft2/day. Fig. 4.2 shows the variation. of the
displacements at surface node A! with time and Fig. 4.3 the variation of
excess porewater pressure along the axis of the column at various times.
Uniformly distributed vertical load is assumed to be applied on the
surface of a saturated homogeneous elastic soil deposits uderlain by
impervious base. This corresponds to a classical one dimensional
consolidation problem. Theoretical solution for this problem was presented
by Terzaghi �921!. For the analysis by the developed program, a soil
column, 7ft. high, and 1 ft. wide, is descretized as shown in Fig. 4.1. Thematerial properties are as follows:
Good agreements between the finite element results and analytical resultscan be seen.
A uniform strip load applied on a Quid-saturated homogeneous
elasto-porous half space is considered next. This problem has been solved
analytically by SchifFman et al. �969!. Finite element descretization of the
problem is shown in Fig. 4.4 and the material properties used are
Young's modulus K! = 1000 KN/m2
Poison's ratio v! = 0.
Unit weight of water p~! = 1000 kg/m3
The time factor T in this problem is defined as
�-~!
where d = half of the width of loaded area; and
2GI<
Pf �.3!
42 ~m:mac Problems
43
with 6 = shear modulus. Fig. 4.5 shows the computed variation of excess
pore pressure, beneath the center of loaded area, at T = 0.1. Good
agreements between the finite element results and analytical results can beseen.
A uniformly distributed vertical load is applied over the surface of a
homogeneous fluid-saturated elasto-porous half space. The following two
different loading time histories, step function and triangular impulse time
histories, are considered as shown in Fig. 4.6. Analytical solutions for
those cases were presented by Simon et al. �984!. In the 6nite element
computation, the maximum intensity of the load is 10 units and material
properties are as follow:
Young's modul~s K! = 3000 units
Poisson's ratio {v! = 0.2
Density of fluid {pf! = 0.2977
Density of solid p~! = 0.3101
Porosity n! = 0.333
Bulk density {p! = 0.306
CoeKcient of permeability k! = 0.004883
Bulk stiBness of solid grain K,! = 0.5005 x 104
Bulk stiffness of fluid +! = 0.6106 x 105
The responses are computed for the step loading time history by
using the finite element descretization shown in Fig. 4.7 with soil depth = 60units. The time step ht! is 0.002 time units. Figs. 4.8 and 4.9 show
respectively the comparisons of the solid and. fluid displacements at the
surface node A!. Figs. 4.10 and 4.11 show respectively the variations of
solid and fluid displacements along the depth at t = 0.06 time units.
The responses are also computed for the triangular impulse loading
time history by using the finite element descretization as shown in Fig. 4.7
with soil depth = 120 units. Material properties are same as those
aforementioned except K, = ~ for the present problem. The loadingduration = 2 d to! is 0.021 time units. The time step ht! is 0.002 time units.
Fig 4. 12 sho~s the variation of displacement of solid and Fig. 4. 13 showsvariation of f1uid displacement at surface node A! with time. Variations of
the responses along the depth at t = 0.12 units are also shown in Fig. 4.14through 4.17 for soiM and Quid phases.
5. ZXAiVIPLE OF COMPUTED BEHAVIOR OF WATERFRONT SHZETPILE WALL clL'B JKCTED TO ErMTHQUAKE SKARBNG
In 1983, Nihonkai Chubu Earthquake of magnitude 7.7 hit northern
part of Japan. The earthquake caused damages to quay walls at the Akita
Port located about 100 km from the epicenter. Damages were associated
with liquefaction in backfill sand. Fig. 5.1 shows a cross section view of a
sheet pile of Oohama No. 2 wharf, at which the water depth is 10 m. This
sheet pile was displaced about 1.1 m to 1.8m towards the sea and was
cracked due to excessive moment at about 4m above the sea bed. Sand boils
and settlexnents wexe observed at the apron, indicating liquefaction in
bacldill induced during the earthquake shaking.
Based on information given by Tsuchida, et al. �985!, the soil at the
sheet pile is divided. into four homogeneous layers as shown in Fig. 5.1. Theproperties of each layer are G~~ = 65030 kpa, max. bulk modulus of soil
skeleton = 173400 kpa, P = 370, Kp = 2x106 kpa. The sheet pile is FSP-VEg type
of which second moment of area = 8.6xl0-4, cross section area = 0.306 m2
and density = 7.5 tfm3. The 6nite element mesh used is shown in Fig. 5.2.
The tie bar is idealized as massless beam elexnents and hinge connections
are assumed at the connections to sheet pile and anchor piles. Two anchor
piles and sheet pile are idealized by beam elements. The top ends of two
anchor piles are capped with a rigid mass.
Earthquake ground motions, recorded at nonlique6ed ground. at the
Akita Port, were used to determine input xnotions. The maximum
accelerations recorded are 190 gal and 205 gal in the NS and EW
seconds corresponds to the end of shaking. The stress due to the
maximum bending computed is 320,000 kpa whereas the failure strength of
steel of the sheet pile is 300,000 kpa. Seismic eFects significantly increasethe earth pressure and bending moment.
48
Anzo, Z., 1936, "Dynamic Water Pressure against Retaining Walls duringEarthquake," in Japanese!. Proc. 3rd Aaaual Meeting of Japanese Societyof Civil Engineers.
Ayala, G., Rorno, M.P., and Gomez, R., 1985,"Earthquake Analysis ofFlexible Retaining Walls," Proc. 5th Int. con. Numerical Methods inGeomechanics, Nagoya.
Bolton, M.D. aad Steedmaa, R.S., 1985,"Modelling the Seismic Resistanceof Retaining Structures, " Proc. 11th Int. Conf. Soil Mechanics andFoundation Engrg., Vol. 4, pp. 1845-1848.
Clough, G.W. and Duncan, J.M., 1971, "Finite Element Analysis ofRetaining Wall Behavior," J. Soil Mechaaics and Foundation Engrg.,ASCE, Vol.97, SM 12.
Goodmaa, R.E., Taylor, R.L., and Brekke, T.L., 1968, "A Model for theMechanics of Jointed Rock," J. Soil Mechanics and. Foundation Engrg.,Vol. 94, SM3.
Ishibashi, I., Maisuzawa, H., and Kawamura, M., 1985,"GenerahzedApparent Seismic Coef5cient for Dynamic Lateral Earth PressureDetermination, Proc. 2nd Int. Conf. Soil Dynamics and EarthquakeEngineering, Southampton, Vol. 6, pp. 33-42.
Ishii, Y., Arai, H., and. Tsuchida, H., 1960, "Material Earth Pressure in anEarthquake," Proc. 2nd World Conf. Earthquake Engrg, Tokyo, Japan.
Jacobsen, L.S., 1939, Described in The Kentucky Project, Technical ReportNo. 13, Tennessee Valley Authority, 1951.
Ku.ralowicz, Z. aad Tejchman, A., 1984, "Interaction between Flexible SheetPiling in Cohesioaless Soil," Proc. 6th Conf. Soil Mechanics andFoundation Engrg., New Zealand.
Matsuo, H., 1941, "Experimental Study on the Distribution of EarthPressure Actiag on a Vertical Wall duriag Earthquake Pressure Acting ona Vertical Wall duriag Earthquake, J. Japaaese Society of Civil Engineers,Vol. 27, No. 2.
Matsuo, H. and Ohara, S., 1960, "Lateral Earth Pressure and. Stability ofQuay Walls during Earthquakes," Proc. 3rd World Conf. EarthquakeEngrg., New Zealand.
Matsuo, H. and Ohara, S., 1965, "Dynamic Porewater Pressure Acting onQuay Walls during Earthquakes," Proc. 3rd World Conf. EarthquakeEngineering, New Zealand.
The Minister of Transportation, 1964, "Damages of Ports and HarborsCaused by the Niigata Earthquake," Japanese!.
Mononobe, N., 1929, "Earthquake-Proof Construction of Masnary Dams,"Proc. World Engineering Conf., Vol. 9, p. 275.
Mononobe, N. and Matsuo, H., 1929, "On the Determination of EarthPressure during Earthquakes," Proc. Engineering Conf., Vol. 9, p. 176.
Murphy, V.A., 1960, "The Effect of Ground Characteristics on the AseismicDesign of Structures," Proc. 2nd World Conf. Earthquake Engrg., Vol. 1,pp. 231-247.
Okabe, S., 1926, "General Theory of Earth Pressure," J. Japanese Society ofCivil Engineers, Vol. 12, No. 1.
Potts, D.M. and Fourie, A.B., 1986, A Numerical Study of the ZQ'ects of WallDeformation on Earth Pressures. Int. J. Numerical and AnalyticalMethods in Geomechanics, Vol. 10, pp. 383-405.
Prakash, S. and Basavanna, B.M., 1969, "Earth Pressure DistributionBehind Retaining Walls during Earthquake," Proc. 4th WorM ConfEarthquake Engrg., Santiago, Chile.
Saabzevari, A. and Ghaahramani, A., 1974, "Dynamic Passive EarthPressure Problem., J. Geotechnical Kngrg., ASCE, Vol. 100, GTI, pp. 15-30.
Schifman, R.L., Chen, A.T. and Jordan, J.C., 1969, "An Analysis ofConsolidation Theories," Int. J. Soil Mechanics and FoundationEngineering, ASCE, Vol. 95, pp. 285-312.
Seed, H.B. and Whitman, R.V., 1970, "Design of Earth RetainingStructures for Dynamic Loads," Lateral Stresses in the Ground and Designof Earth-Retaining Structures, ASCE.
Simon, B.R., Zienkiewicz, O.C. and Paul, D.K, 1984, "An AnalyticalSolution for Transient Response of Saturated. Porous Elastic Solid, Int. J.Numerical and Analytical Methods in Geomechanics, Vol. 8, pp. 381-398.
Tajimi, H. 1973, Dynamic Earth Pressure on Basement Wali," Proc. 5thWorld Conf. Earthquake Engrg., Rome, Italy.
Terzaghi, K, 1925, "Principle of Soil Mechanics," Engrg. News Record.
50
Towhata, I. and Islam, S., 1987, "Prediction of Lateral Displacement ofAnchored Bulkheads Induced by Seismic Liquefaction," J. Soils andFoundation, Vol. 27, No.4, pp.137-147.
Tsuchida, H. et al., 1985, "Damage to Port Structures by the 1983 Nipponkai-Chubu Earthquake," Technical Note of the Port and Harbor ResearchInstitute, No. 511, p. 447
Zienkeiewicz, O.C. and Shiomi, T., 1984, "Dynamic Behavior of SaturatedPorous Media; The Generalized Biot Formulation and Its NumericalSolution," Int. J. Numerical and Analytical Methods in Geomechanics,Vol. 8, pp. 71-96.
+W0
4 m ~CO g!
oHW
q
O
' Fig. 2.1 Jaint Element
IFig. 2.2 Stress-Strain Relationship at Soil-WaH Interface
contact ~ ~ seper ation
<ns
OW go~
p =>m =>nCQ
O
'C
C!CO
j X~ XQ~8
+A
Q '4
B~k
O
O bnFG
M
T = 0.01
10050
Excess Pore Pressure psf!
Fig. 4.3 Variations of Excess Pore Pressure with Depthat Various Times Static 1-D problem!
0 0
alyticalu tion
I CQO 8
8
~
Q '49-8~
.8-
4
V
r j
Fig. 4.6 Loading Time Histories
qo
qp
q t!
0
q t!
0 0.012 units
3U3
4
4 O
p -X~ -Xg
~ 8'5 2O O
aA
~8g84
g~
88OPI
OV
0
'0 QCf}
O
-0.02
O cf
a
-0.04 .
0 0.05 0.15
Time
Fig. 4.8 Variation of Displacement of Solid at Surface with Time Step Function Loading!
xl 0-2
0.6
0
0.050 O,l 0
T1m e
Fig. 4.9 Variation of Displacement of Fluid at Surface with Time Step Function Loading!
x10-2
0.20 0.1 0.3
20
40
60
Fig. 4.11 Variation of Displacement of Fluid with Depth at t = 0.06 Step Function Loading!
-0.1
0
Disp1acement of Fluid
x10-2
0
-0.4
0.05 0.10 0.15
Time
Fig. 4.12 Variation of Displacement of Solid at Surface with Time Triangular Impulse Loading!
0.3
0
0.1 50.05 0.10
Time
Fig. 4.13 Variation of Displacement of Fluid at Surface with Time Triangular Impulse Loading!
Total Stress
100
40
120
Fig. 4.16 Variation of Total Stress with Depth at t = 0.12 Triangular Impulse Loading!
-. Pore Pressure '
-5 10 150
40
80
1ZO
Fig. 4.17 Variation of Excess Pore Pressure with Depth at4 = 0.12 Triangu1ar Impulse Loading!
.9
0
Q :8K
C!
C>
C!
LQ
P.
A 8
8 8 OO
cm!node A
0
-43
172
0
-172
. 207
0
-207
10
Tim e sec.!
, Fig. 5.4 Horizontal Displacement Time Histories at Various Locations
em!
194
0
-194
147
0
-147
1510
Tim e sec.!
15.8
0
Fig. 5.5 Vertical Displacement Time Histories at Various Locations
gal!
Fig. 5.6 Horizontal Acceleration Time Histories at Various Locations
189
0
-189,
218
0
-218
147
-147
0
Tim e Sec.!
10
node A
'I
node H
~ nodeEI
clem ent B27.9
0
-27.9
81.8
0
-81.8
91.7
-91.7
48.8
0
-48.8 !10
Time sec.!
Fig. 5.7 Excess Pore Pressure Time Histories at Various Locations
ha
K A
S OCQ
t
kpa m!1180
clem e
0
-1180
100
Time sec.!
Fig. 5.9 Bending Moment Time History at 6 m below the Sea Level
kpa!2000-200
P ressure on the % all
Fig. 5.11 Pressure Acting on Sheet Pile before andat 15 Seconds of Earthquake Shaking