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     Missouri University of Science and Technology 

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    Piles Under Dynamic LoadsM. Novak 

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    Proceedings: Second International Conference on Recent Advances

    In

    Geotechnical Earthquake Engineering and Soli Dynamics

    March 11-1.5 1991 St. Louis Missouri Paper No. SOA14

    Piles Under Dynamic Loads

    M. Novak

    Professor of ivil Engineering The University of Western Ontario

    London Ontario Canada

    SYNOPSIS The

    paper

    deals with some of the more recent developments in

    p i l e

    dynamics. It reviews

    the progress in

    the ana lys i s

    of s ing le

    pi les and p i l e groups, f ie ld as well as l abora tory exper i

    ments and so i l -p i l e - s t ruc ture in te r ac t ion . The in f luence o f p i l e - so i l i n t e r face i s discussed and

    extensive

    references

    are

    given.

    INTRODUCTION

    Pi l es have been used

    for

    hundreds

    of

    years bu t

    the

    l a s t twenty

    years

    or

    so

    have

    seen

    a

    remarkable increase in i n t e r e s t

    in

    p i l e dynamics.

    There

    are a

    few reasons

    for

    t h i s : good s i t e s

    which

    do not requi re

    pi les

    are

    ge t t ing

    scarcer

    and thus p i l i ng

    i s

    used

    more

    widely; new

    important areas of appl icat ion have

    emerged,

    for

    example of fshore

    towers and

    nuclear powerplants;

    pi les have repea tedly f a i led

    in earthquakes or

    were damaged; and f ina l ly , dynamics

    of

    shal low

    foundations

    has reached a poin t

    of sa t i s f ac tory

    understanding

    thus sh i f t ing

    research i n t e res t s to

    les s understood foundat ion types . The aim of the

    s tudies i s to increase the sa fe ty

    of

    the pi l e s

    and the s t ruc tures they support

    and

    to

    be t t e r

    understand

    the

    in te r ac t ion between the pi l e s and

    the

    s t ruc tures

    under both c r i t i c a l and

    opera t iona l condi t ions .

    The

    damage to

    pi l e s may re su l t

    from

    a few

    causes

    such as v ib ra t ion ef f ec t s , l i quefac t ion ,

    and

    embankment movements. A comprehensive survey

    of

    pi l e

    damage

    during earthquakes in

    Japan

    was

    presented

    by

    Mizuno (1987) but damage to pi l e s

    also

    occurred

    in

    the

    Alaska earthquake

    of

    1964,

    the

    Mexico City

    earthquake

    of

    1985

    and the Lorna

    Pr ie ta earthquake

    of

    1989.

    Pi le

    behavior

    i s ,

    of

    course,

    very

    complex

    and

    t h i s might have lead Terzaghi and Peck (1967) to

    s t a t e tha t heore t ica l

    refinements in

    deal ing

    with pi l e problems

    are

    completely out o f

    place

    and can be

    sa fe ly ignored .

    For tuna te ly , not everybody got

    discouraged

    by

    t h i s

    pessimist ic

    eva lua t ion and

    a

    number of

    ana ly t ica l

    and

    numerical approaches

    to

    the

    analysis

    o f p i l e

    dynamic behavior have been

    developed.

    These

    approaches

    provided

    a

    much

    sounder theore t ica l

    basis for

    p i l e

    design than

    the equiva lent cant i l ever concept

    or o ther

    purely

    empir ical methods

    which

    dominated

    the

    f i e ld for

    decades. Never theless , some

    d i f fe rences

    between

    the

    var ious theore t ica l

    approaches

    ex i s t

    and the

    experiments repor ted are sometimes inconclusive;

    also ,

    some uncer ta in t ie s

    are inev i t ab le

    when

    applying an

    i dea l i zed theory to f i e ld condi t ions .

    Thus, it may be usefu l

    to

    review

    some of

    the

    433

    approaches

    in

    order t h a t

    we may

    examine

    t he

    di f ferences

    among

    them and

    summarize

    what

    can be

    learned from experiments and f i e ld observa t ions .

    There

    are

    di f f e r en t dynamic

    loads

    t h a t can ac t

    on pi l e s : earthquake

    forces ,

    wave forces,

    wind

    forces , machine unbalances

    e tc .

    Here, t he

    emphasis

    is pr imar i ly on condi t ions relevant

    to

    earthquake loading. Dealt with are p roper t i es

    and behavior

    of

    s ing le p i l e s and p i l e groups,

    in te r ac t ion with

    the

    cap,

    p i l e

    experiments ,

    p i l e

    s t ruc ture in te r ac t ion

    and a

    few

    other

    top ics .

    The

    subject o f pi l e dynamics received a

    comprehensive

    t reatment

    in

    the

    s t a t e - o f - t h e - a r t

    repor t by Taj imi ( 1977) , covering developments up

    to

    1977, and in a

    few

    spec ia l volumes, i . e . De

    Beer

    e t

    al .

    (1977), O Nei l l

    and

    Dobry (1980),

    Nogami

    (1987)

    and

    Prakash

    and

    Sharma

    (1990). A

    number o f papers

    on pi l e s were

    presen ted to t h i s

    conference.

    These are l i s t ed together

    a t the end

    of

    the

    References.

    Among

    the

    spec ia l

    areas

    of

    pi l e dynamics not considered

    here

    are i n t egr i ty

    t e s t i ng and p i l e dr iv ing . Recent data on

    these

    subjects can be found in

    Fel len ius

    (1988).

    So

    many

    papers have

    been published

    on

    p i l e dynamics

    s ince

    Taj imi s

    (1977) s t a t e - o f - t h e - a r t

    r epo r t

    t ha t it i s

    impossible

    to re fe r

    to

    a l l

    of

    them in

    t h i s

    r epo r t

    of

    l imi ted

    scope. The au thor

    t r u s t s

    tha t

    the readers

    wi l l understand t h i s .

    SINGLE PILES

    The e a r l i e s t systemat ic , t he o r e t i c a l

    s tudies

    of

    dynamic so i l - p i l e in te r ac t ion are due to Parmelee

    e t

    a l . (1964),

    Tajimi

    (1966), Penzien (1970),

    Novak (1974)

    and a

    few

    others . Parmelee (1964)

    and

    Penzien (1970) employed a

    non- l inear disc re te

    model

    and

    a

    s t a t i c

    theory

    to

    descr ibe

    the

    dynamic

    e l a s t i c s t r e s s and

    displacement f ie lds .

    Tajimi

    (1966) used

    a

    l i nea r viscoe las t ic s t ra tum of t he

    Kelvin-Voigt type to model the so i l and in

    h i s

    analysis of

    the

    hor izontal

    response neglected

    t he

    ver t i ca l component of

    the

    so i l

    motion.

    Novak

    (1974)

    assumed l i nea r i ty and an e l a s t i c so i l

    layer

    composed

    of

    independent in f in i te s imal ly

    th in hor izontal layers

    extending

    t o in f in i ty .

    The di f fe ren t

    approaches

    formulated

    and the data

    they

    yie ld

    are

    br ie f ly

    discussed

    below.

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    5.5

    4.5

    (a)

    ~ - - ~ 2 5 ~ - - - = 5 ~ 0 - - ~ 7 ~ 5 ~ - - ~ ~ o ~ o ~ ~ L - I ~ d ~

    12

    10

    6

    4

    Floating Piles

    v =

    0.5

    ·

    .-·

    . - ·

    .

    Ep/E

    5

    =

    1000

    /

    Present ( 50 Elements l

    Poulos 10 Elements)

    · · · · Salinera (

    >

    20 Elements l

    X • X

    Rajapakse a Shah

    Ep/E

    5

    = 100

    ---

    --

    ---

      b)

    z ~ - - ~ 2 5 ~ - - - - ~ 5 ~ 0 - - - - ~ 7 ~ 5 - - - - ~ ~ o ~ o ~ ~

    L/d

    Figure 4 Comparison

    of

    s t a t i c axial p i l e

    s t i f f n e s s

    calcu lated

    by d i f f e r e n t au thors

    for

    homogeneous so i l :

    (a)

    - endbearing pi l e s , (b) -

    f loa t ing

    p i l e s (Present

    data by

    El

    Sharnouby and

    Novak, 1990)

    J

    UJ

    0

    >

    1-

      ;

    a.

    ;

    30

    ·

    .

    . . .

    0 33

    p

    ·

    T£5T PILE

    2

    2r

    2.41N.

    (6.1 em I

    I • 0.000032 FT

    4

    27.6 cm

    4

    1

    l;r.

    77.9

    G Z)

    (a )

    (b )

    z

    Figure 6 Schematic of p i l e separa t ion

    and

    so i l

    modulus

    reduct ion

    towards ground sur face

    Observat ions

    of t h i s

    kind

    l ead to

    the development

    of

    approaches

    be t t e r

    su i ted for nonhomogeneous

    so i l s .

    A

    s ign i f ican t

    improvement in the f i n i t e

    element

    model

    was

    formulated by Roesset and h i s

    co-workers

    (Blaney

    e t a l . ,

    1976;

    Roesset

    Angelides,

    1979)

    who placed

    t he cons i s t en t ,

    f requency

    dependent boundary, derived

    by

    Kausel

    e t

    a l (1975), d i r e c t l y t o t he p i l e or out s ide the

    cy l ind r i ca l

    f i n i t e element zone around the pi l e .

    This approach

    was

    then used

    by

    Krishnan e t a l .

    (1983)

    and by

    Gazetas (1984)

    in

    t h e i r extens ive

    parametr ic

    s tud ies .

    S ign i f i can t fu r ther progress was

    made

    by Kaynia

    (1982a,b) and Kaynia and Kausel (1982,

    1990)

    who

    based t he i r so lu t ion of p i l e s

    in

    genera l ly

    layered media

    on the. formulat ion of

    d i sp lace

    ment

    f ie lds

    due

    to uniformly

    dis t r ibu ted

    forces

    on cy l ind r i ca l sur faces (so ca l l ed bar r e l

    load) .

    (This

    so lu t ion wi l l

    be

    discussed in

    more d e t a i l

    in

    the

    paragraph on p i l e

    groups.)

    Baner jee

    and Sen (

    1987)

    presented bounda:y

    element

    so lu t ion

    for

    p i l e s embedded 1n

    a

    sem1-

    i n f i n i t e nonhomogeneous so i l

    in

    which

    the

    so i l

    modulus, E

    5

    , var i es l i nea r ly with

    depth, z.

    Baner jee

    and Sen s re su l t s suggest

    tha t ,

    unl ike

    in layered so i l s , the

    f requency

    var i a t ions of the

    impedance

    funct ions,

    normal ized

    by s t a t i c s t i f f

    ness, are qu i t e smooth and are

    af fec ted

    very

    little by so i l nonhomogeneity.

    The ac tua l

    magni

    tude of the s t i f fness and damping diminishes with

    E

    5

    (0) , however.

    ,

    ~ ~ ~ ~ ~ ~ ~ ~ ~ ~

    m m

    w

    w

    A

    few

    other methods

    su i tab le for l i ne a r genera l ly

    layered media

    use

    a semi-ana ly t i ca l f i n i t e e le

    ment approach.

    These methods t r ea t

    the wave pro

    paga t ion

    in the

    hor izonta l di r ec t ion ana ly t ica l ly

    and in the ver t i ca l di r ec t ion employ f i n i t e

    e l e

    ment

    i dea l i za t ion including aux i l i a ry

    sublayers .

    The p i l e

    is

    modelled by

    beam elements .

    One of

    the

    advantages

    of

    t h i s

    approach i s

    t ha t

    it

    may

    avoid the mathemat ical i l l - condi t ion ing r esu l t ing

    from the

    large

    magnitude of

    Lame s

    cons tant ,

    for so i l Poisson s ra t io ,

    v ,

    approaching 0. 5.

    Solutions o f

    t h i s

    type were

    formulated by

    Tajimi

    and Shimomura (1976) , Shimizu

    e t a l .

    (1977) ,

    Waas and Hartmann (1981,

    1984)

    and Mizuhata and

    Kusakabe

    (1984).

    60

    FREQUENCY (CPS)

    Figure 5 Comparison

    of

    experimental

    hor izontal

    response

    of

    s t ee l

    t e s t

    p i l e with theore t ica l

    predict ions

    (Novak

    and Sheta,

    1982)

    2436

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    An approximate ana ly t ica l so lu t ion based on t he

    extension

    of

    the Novak and

    Nogami (1977) approach

    was formulated for layered media by Takemiya and

    Yamada (1981).

    A much s impler and

    very v e r sa t i l e

    so lu t ion ,

    p a r t i c u l a r l y well

    sui ed for

    high f requencies ,

    was formulated

    by

    Novak

    and

    Aboul-Ella (1978a,b)

    who

    extended

    the plane

    s t r a i n approach

    to include

    layered

    media and

    incorporated t in

    the

    code

    PILAY.

    This

    code

    was

    used l a t e r by

    Novak

    and

    El

    Sharnouby

    (1983)

    to generate design char t s

    and

    t ab l es

    for parabol ic

    so i l p rof i l e s , as well as

    homogeneous

    ones. With t h i s approach, and

    assuming a parabol ic s o i l prof i l e ,

    with an

    al lowance

    for

    p i l e

    separat ion in the form of

    a

    small

    f ree length,

    very sa t i s fac tory agreement

    with

    the

    theory was obtained as ind icated by

    curve c in

    Fig. 5.

    Roesset e t al . (1986) a l so

    found

    t he plane s t r a in

    approach to

    work very

    well

    for

    high f requencies . For very low f requencies ,

    an

    adjustment

    to the plane s t r a in

    so i l

    react ion

    i s

    made

    for the

    ver t i ca l

    and hor izontal

    d i r ec t ions as d iscussed

    in

    Novak

    and

    El

    Sharnouby

    (1983)

    and implemented in the code

    PILAY. The

    plane s t r a in

    approach

    works

    well

    for

    high

    frequencies because, in a l ayer , e l a s t i c waves

    tend

    to

    propagate

    more and more hor i zon ta l ly as

    the

    f requency

    increases ,

    l i ke

    in

    a

    wave

    guide.

    The sens i t iv i ty

    of

    t he

    response to

    p i l e separa

    t i on

    and

    f ree l ength

    shows

    when

    eva lua t ing

    most

    experiments . The predict ion

    of the separat ion

    leng th i s d i f f i cu l t and

    only

    empi r ica l

    sugges

    t ions

    can

    be

    made

    a t

    t h i s

    t ime.

    For small ampli

    tudes, 6 , El-Marsafawi e t a l . (1990) observed t he

    fol lowing approximate r e la t ionsh ip

    for

    p i l e

    separa t ion l ength , L

    8

    :

    Ls

    d

    260 , 0.001 5 5

    0.005 2)

    For l a rge r displacements, a large

    separat ion

    length may

    be

    needed

    (Han

    and

    Novak,

    1988) .

    More

    data

    on

    the separat ion

    e f fec t

    wi l l

    be

    given

    in

    the paragraph on nonl inear response.

    As

    for poss ib le deviat ions

    o f the theore t ica l

    assumpt ions from

    r ea l i t y , p i l e def ic ienc ies may

    also

    have a profound e f fec t . This i s shown by

    Wu

    e t a l . (1991)

    who,

    in t h e i r paper to t h i s confe

    rence,

    examine the in f luence of p i l e necking

    using a

    combinat ion

    of

    the

    BEM and FEM

    adial nonhomogeneity

    While the cons idera t ion of a f ree separat ion

    leng th in the

    ana ly s i s

    may produce

    the reduct ion

    in both p i l e s t i f f n e s s and damping of ten observed

    in

    experiments , a b e t t e r measure to

    t h i s e f fec t ,

    or

    a complementary

    one,

    may be to account

    for

    so i l

    nonhomogeneity in

    the

    rad ia l

    di r ec t ion . A

    simple

    way

    of

    doing

    t h i s

    i s

    to

    assume

    a

    weak,

    cyl indr ica l

    boundary

    zone around the p i l e (Fig.

    7).

    The

    zone i s

    homogeneous

    and features

    a so i l

    shear modulus, G., smal le r than t ha t

    of

    the outer

    zone

    and

    a

    l r g e ~ mater ia l damping.

    The

    purpose

    of such a zone is to account in a very approxi

    mate

    way

    for

    so i l

    non l inear i ty

    in

    the region

    of

    the h ighest

    s t re sses , p i l e

    separat ion ,

    s l ippage

    and

    o ther def i c i enc ies o f the p i l e - s o i l

    inter face . Such a zone was proposed

    by

    Novak

    and

    Sheta (1980). In

    t h e i r

    plane

    s t r a in so lu t ion ,

    the mass

    of

    the boundary zone was neglec ted in

    ·. G,p , v

    Figure

    Cyl indr ica l boundary zone around p i l e

    order to preven t wave re f l ec t ions from t he

    f i c t i t i o u s inter face between the

    cyl indr ica l

    zone

    and t he

    outer reg ion . These r e f lec t ions occur

    with nonzero

    weak zone mass, p . and re su l t in

    undes i rab le undulations in bot h s t i f f n e s s and

    damping

    of

    the

    composite medium. This i s

    exemplified in Fig. 8 in which a and

    are

    {b)

    ~ ~ ~ ~ ~ ~ ~ ~ ~

    0 2 3

    requency

    0; :

    r

    0

    W/V;

    Figure 8

    Dimensionless

    ver t i ca l impedances

    of

    composi te medium with P = and

    tjr

    0

    = 1.0 s o i l

    damping r a t i o = 0.05)

    nondimensional s t i f fness

    and

    damping cons tan t s

    of the

    composite

    medium r espec t ive ly . These

    undulat ions can make

    the

    so lu t ion with

    P 1

    0

    ac tua l ly l e s s su i tab le

    for

    prac t i ca l

    appl icat ions

    (Novak

    and Han,

    1990).

    The di f f icu l ty

    with wave

    r e f lec t ions can be avoided by providing

    for

    a

    continuous

    t r ans i t ion of s t re sses from the inner

    zone

    to the ou ter

    region. Such a

    so lu t ion was

    explored

    by Lakshmanan and Minai (1981), Dotson

    and

    Veletsos

    1990) and

    Mizuhata and

    Kusakabe

    (1984).

    The

    l a t t e r au thors found t ha t even with

    the

    weak

    zone, the

    experimental

    resonance

    ampli tude measured on a

    43.2

    m

    long

    p i l e was f ive

    t imes l a rge r

    than the

    theore t ica l value while

    the

    resonance frequency was predic ted

    qui te wel l .

    This i s cons i s ten t

    with

    other observat ions and

    i nd ica t ive o f t he need to

    account

    for p i l e

    separat ion .

    2437

    Wolf and

    Weber

    (1986)

    conducted

    a more r igorous

    study

    of

    the

    effect

    of

    soil tension

    exclusion,

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    also assuming the c i rcu la r cavi ty in the

    unbounded

    th in

    l y ~

    plane s t r a in)

    . They

    found

    t ha t so i l

    separatidn hardly a f fec t s hor izontal

    s t i f fness , lS,, but

    reduces

    damping, ch, by more

    than 50

    per cent

    Fig.

    9b), a r esu l t

    qui te

    s imilar t o tha t

    of Novak and Sheta 1980). In

    addi t ion ,

    i f shear i s

    el iminated

    and hence

    s l ipp ing i s allowed in the zone

    of

    contact ,

    s t i f fness i s also s t rongly reduced Fig. 9c). In

    Fig. 9,

    the

    l i nea r case

    a)

    indicates the

    analysis

    with

    tension

    allowed.

    The

    s i ze

    of

    the

    contact

    area appears

    to be

    of 1 i

    t t l e

    ef fec t .

    Many other authors s tudied the

    in te r f ace

    behavior.

    Among

    the more recent ones

    are Mamoon

    1990) and

    He

    1990). However, when applying

    the

    var ious plane

    s t r a in

    approaches to

    the

    in te r f ace ,

    the

    var ia t ion

    with depth i s

    a

    problem

    for

    which

    very l i t t l e

    guidance

    is avai lable .

    Linear

    ,,,,,,,,.,,,

    ~

    4.28

    13.23

    a)

    Shear

    Slipping

    [) D

    QG)

    4.17

    6.42

    b)

    2.32

    2.60

    c)

    Figure 9

    separation

    v=0.48)

    Effec t of

    elimination

    of

    tension

    in

    zone Wolf Weber 1986; a

    0

    =0. 629,

    Recognizing

    the

    separa t ion

    e f fec t and allowing

    for

    t

    in an

    approximate

    way, a reasonable

    agreement

    between the theore t ica l

    re su l t s

    and

    experiments can be

    obtained. This i s exemplif ied

    in Fig. 10 comparing the t heore t i ca l and

    experimental responses of a concrete p i l e 7.5 m

    in length

    and

    0.

    32 m

    in dia . The

    so i l

    was

    mul t i l ayered and

    a

    cyl indr ica l

    weak zone was

    assumed when

    calcula t ing the

    response using the

    code

    DYNA3.

    In t h i s code, the weak zone i s

    analyzed as massless but i t s mass i s added to

    tha t

    of

    the

    pi le

    in fu l l or in par t .

    Simila r

    t e s t s and comparisons were repor ted by Gle

    1981), Woods

    1984)

    and a number of others .

    Nonlinear

    Response

    of Single

    Pi les

    The theor ies

    discussed thus

    far

    are

    essen t i a l ly

    l inea r and thus qui te adequate

    for

    small

    displacements.

    At large displacements, pi les

    behave in

    a

    nonl inear

    fashion

    because

    of

    so i l

    nonlinear i ty

    a t

    high s t r a in ,

    p i l e

    separat ion

    gapping), s l ippage and f r ic t ion .

    To

    incorpora te

    these

    factors

    in to

    a

    continuum

    theory i s

    extremely d i f f i cu l t and

    therefore , lumped

    mass

    models are most often used when nonl inear

    analysis s required. Such models employed by

    2438

    1.1

    1 .3

    1 .2

    1.1

    1.0

    ....

    o.

    a

    c..

    o.

    E

    o.

    G

    :

    0. 5

    '

    ...

    0. 1

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    ,;oil res is tance-def lect ion relat ionships known as

    p-y curves and t -x curves have been recommended

    in the

    l i t e ra ture .

    For appl icat ions in offshore

    s t ruc tu res the American

    Petroleum

    I n s t i t u t e

    (1986) spec i f i es t he p-y curves

    for

    c lay as well

    as

    sand

    making

    a dif ference between s t a t i c

    loading

    and cycl ic

    loading. Extensive data on

    the

    p-y curves

    and

    nonl inear p i l e response were

    obtained by Yan

    (1990)

    using

    model pi les

    and the

    hydraulic gradient s imi l i tude

    method to

    reproduce

    prototype

    condit ions. An

    example of Yan's

    resul ts

    i s shown

    in

    Fig. 12.

    Notice the

    narrowing

    and p ar t i a l

    l inea r iza t ion of the

    hysteres is

    loop with

    the

    number of cyc les ;

    t h i s

    t rend

    increases

    with

    depth.

    Pile Deflection -

    y

    mm)

    Figure 12 Example of p-y curve under cyc l i c

    loading (Yan, 1990)

    Cyclic

    loading is

    def ined as r e pe t i t i ve

    loading

    with very low

    f requency so t ha t no s ign i f ican t

    i ne r t i a

    fo rces

    and rad iat ion damping

    ar i se .

    t

    provides bas ic ins ight in to the mater ia l

    degradation

    due to

    so i l p l a s t i c i t y and mechanic

    degradation due

    to gapping

    assoc ia ted with large

    displacements .

    Many s tudies were devoted to t h i s

    subjec t but only a

    few

    may be mentioned here .

    Trochanis

    e t

    a l . (1988)

    found

    theore t ica l ly a

    dramatic

    decrease

    in

    p i l e s t i f f n e s s due to

    gapping.

    Morrison and Reese (1988)

    conducted

    extensive fu l l sca l e

    invest igat ion

    of pi l e s and

    pi l e

    groups. To

    t h i s

    conference,

    Purkayastha

    and

    Dey

    (1991)

    repor t

    on t he i r experimental s tudy of

    the degradation of ver t i ca l s t i f fness .

    Summarizing t he i r observat ions , Swan and Poulos

    (1982)

    postu late

    t h a t

    during

    cyc l ic

    l a t e r a l

    loading the two forms of degradation lead

    to

    the

    increase in pi l e def l ec t ion

    and

    bending s t r es ses ;

    but i f t h i s degradation s t a b i l i z e s the p i l e i s

    sa id

    to

    shakedown

    to

    a

    s t a t e

    of

    permanent

    s t r a ins and

    res idual

    s t r es ses

    and

    wil l r eac t

    e las t i ca l ly to any

    fur ther

    cyc l ic loading

    of

    the

    same in tens i ty .

    When the p i l e

    does

    not s t ab i l i ze

    in to an e l a s t i c or i ne las t i c

    response,

    the

    p i l e

    def lect ions continue

    to increase and incremental

    col lapse

    may

    re su l t .

    The two

    s i tua t ions

    are

    depicted in Fig. 13.

    The shakedown phenomenon i s

    favourable

    from

    the

    Stlakodown

    Incrqmczntal

    Collaps.Q

    Figure 13 Pi l e s t ab i l i za t ion (shakedown) and

    incremental

    col lapse

    under cyc l i c

    loading

    with

    constan t amplitude (Swane

    &

    Poulos, 1982)

    poin t

    o f view of the appl icab i l i ty

    of

    the var ious

    l inea r

    theor ies for dynamic response analysis .

    I t

    explains

    why, with adequate adjustments

    par t icu la r ly

    for

    p i l e

    separa t ion

    such

    t heo r i es

    may give

    reasonable r esu l t s

    as in Fig. 10,

    even

    in cases where overa l l s t rong

    nonl inear i ty

    of the

    response

    i s

    c lea r ly manifested.

    Under ver t i ca l

    steady

    s t a t e

    vibrat ion

    a

    s imi la r

    s tab i l i za t ion

    and

    par t i a l l inea r iza t ion

    takes

    place . Figure 14 shows

    the ver t i ca l

    displacement

    2439

    1 5

    ----------------------

    E

    E

    c

    E

    e

    0

    0

    1 0

    0.5

    Q

    >

    0 1 /

    0

    /

    /

    10

    20

    Frequency

    Hz

    )

    e

    s

    14 }

    Measured

    o e

    zs

    Colcuio ed

    Bockbone (]

    30

    Figure 14 Ver t ica l pi l e response

    measured and

    backcalculated for t h ree l eve l s

    of

    exc i ta t ion

    in tens i ty (Han & Novak,

    1988)

    ampli tudes

    measured

    on

    a

    3.38

    m

    long t e s t

    p i l e

    with

    increasing intens i ty

    of

    harmonic exc i ta t ion .

    As

    the

    exc i t a t ion forces grow, t he resonance

    frequencies

    are

    markedly reduced, i nd ica t ing

    s t rong

    nonl inear i ty .

    To the response curves ,

    backbone curves,

    n ,

    can be

    const ructed

    and from

    them the

    p i l e

    res tor ing fo rce-d isp lacement

    relat ionships are estab l i shed

    (Fig.

    15).

    t

    appears t ha t

    each

    response curve

    has

    i t s own

    backbone curve

    and

    corresponding s t i f f n es s

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    -80

    a)

    and

    (b)

    Clay

    Figure 18 Force-displacement r e l a t ionsh ip

    for

    incrementally

    increas ing

    hor izontal load

    (Kishida

    e t a l . , 1985)

    PHe

    Elemeo \

    I

    SoH

    Reaction•

    ~

    t Pile Tip X

    Reactions

    a

    )

    Figure 19 Pi l e model for ver t i ca l v ib ra t ion

    al lowing

    for

    s l ip ,

    nonl inear i ty

    and i n f in i ty of

    the outer zone (Mitwally Novak,

    1988)

    in terms

    of the

    s tandard geo techn ical parameters.

    PILE

    GROUPS

    Pi l es a re usua l ly used in groups and i f they are

    not

    very widely spaced

    they i n t e rac t

    with each

    other

    generat ing phenomena known as p i l e - so i l

    p i l e in te r ac t ion o r group e f fec t s . These ef f ec t s

    have

    a t t r ac ted much

    i n t e res t

    in

    recent years .

    A

    number of

    papers

    on the subject have appeared, a

    few

    exhaustive Ph.D.

    dis se r ta t ions

    were wri t t en

    e.g.

    Kaynia, 1982a; Ostadan,

    1983,

    Mamoon, 1990,

    Hassin i , 1990) and many

    contr ibu t ions

    have been

    made

    to the world conferences on

    earthquake

    engineering

    and

    are

    being presen ted to

    t h i s

    conference.

    Linear Behavior o f

    Pi l e Groups

    Under s t a t i c

    loads, pi l e in te r ac t ion increases

    group set t lement ,

    r ed is t r ibu tes

    t he

    loads

    on

    ind iv idua l pi l e s and

    reduces

    bear ing capac i ty ,

    unless t h i s reduction

    i s

    coun teracted

    by

    densi f icat ion

    of

    the so i l with in the

    group

    due

    to

    p i l e dr iv ing .

    The

    f i r s t

    suggest ion

    of

    t h i s

    kind

    of e f fec t s probably can be a t t r ibu ted to

    Sooysmith

    (1896). The

    i nves t iga t ion

    of

    s t a t i c

    group

    ef f ec t s was

    put

    on

    a

    r a t iona l

    bas i s ,

    re ly ing

    on

    continuum mechanics, by

    Poulos

    (1968,

    1971,

    1979)

    and Butter f ie ld

    and

    Banerjee (1971).

    Extensive data

    on s t a t i c

    group e f fec t s

    are

    avai lab le in

    Poulos

    and Davis

    (1980),

    But te r f ie ld

    and Douglas (1981),

    El

    Sharnouby and Novak (1985,

    1986,

    1990)

    and elsewhere. The s t a t i c data

    are

    usefu l

    even

    to

    those

    in te r es ted in

    dynamics

    because a t low f requencies , and par t i cu la r ly

    below t he fundamental frequency

    of

    a s t ra tum

    (Fig. 2), the dynamic

    s t i f f n e s s

    i s usual ly qui te

    c lose to the s t a t i c s t i f f n e s s .

    Dynamic

    invest igat ions

    of p i l e groups

    are

    more

    recent . The

    techniques

    employed

    are

    ex tensions

    of the

    approaches

    used for s ing le p i l e s and most

    of them are l imi ted to l i nea r in te r ac t ion with no

    al lowance for gapping. The

    methods

    r e ly

    on t he

    ava i l ab i l i ty

    of

    Green 's

    funct ions

    with

    which

    t he

    load t r ans fe r

    from the pi l e sur face to

    so i l

    can

    be

    calcu lated .

    These loading condi t ions ,

    represent ing

    one

    of

    the

    basic d i f ferences between

    var ious approaches,

    range

    from poin t

    loads

    to

    l ine loads ,

    r ing

    loads,

    disk

    loads

    and

    f ina l ly to

    cy l ind r i ca l

    barrel) loads; for

    the

    p i l e

    base,

    disk loads are the ru le .

    Applying

    t h i s loading

    to individual segments in to which t he pi l e i s

    d i sc re t i zed ,

    the

    so i l dynamic displacement f i e ld

    i s estab l i shed ,

    yie ld ing

    the

    so i l dynamic

    f l e x i b i l i t y matr ix ;

    inver t ing the l a t t e r ,

    so i l

    s t i f fness

    matrix

    i s obtained.

    In

    t h i s

    process ,

    the presence of the pi l e

    cavi t i e s

    outs ide

    the

    loaded segment i s

    usua l ly

    ignored,

    which

    impl ies

    t ha t wave sca t te r ing among the pi l e s i s not

    accounted for ,

    and the so i l

    displacements

    are

    calcu lated

    e i the r for t he pi l e axes or as

    averages of

    the

    c i rcumferent ia l va lues . A

    typ ical

    model for t h i s

    ana lys i s i s

    shown in Fig.

    20.

    Then

    the

    so i l

    s t i f f n e s s matrix i s

    combined

    with

    the

    pi l e s t ruc tura l s t i f f n e s s and the

    s o i l

    pi l e system can be analyzed for any type of

    exc i t a t ion .

    Differen t

    au thors

    proposed

    various

    ref inements or

    s imp l i f i ca t ions

    to

    t h i s

    procedure.

    The

    f i r s t

    theore t ica l ana lys i s of p i l e - so i l - p i l e

    i n t e rac t ion was conducted by Wolf and von Arx

    (1978) who employed an

    axisymmetr ic

    f i n i t e

    element formulat ion to es tab l i sh the dynamic

    displacement f i e ld due

    to r ing

    loads . Waas

    and

    Hartmann (

    1981,

    1984)

    formulated

    an

    e f f i c i e n t

    semi-ana ly t i ca l

    method

    which

    uses

    r ing

    loads

    and

    i s well su i t ed for layered media,

    proper ly

    accounting

    for the far

    f ie ld ; the

    layers

    ought

    to

    be

    th in .

    Kaynia

    (1982a,b, 1988)

    and

    Kaynia

    and

    Kausel (1982,

    1990)

    fu r ther

    improved

    the

    accuracy

    by

    combining the cyl indr ica l loads, ac tua l ly a

    boundary element

    formulat ion,

    with t he cons i s t en t

    s t i f f n e s s matrix of layered

    media

    to account for

    the f a r f i e ld . A

    very s imi l a r

    approach

    i s

    employed in

    the

    paper to t h i s conference

    by

    Kobori e t

    a l . (1991) who use

    the

    cyl indr ica l

    244

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     '-'

    ON

    :::>

    ...

    . J

    a..

    I:

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