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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Surface waves in an elastic half spaces: Rayleigh waves

    - Potentials- Free surface boundary conditions- Solutions propagating along the surface, decaying with depth- Lambs problem

    Surface waves in media with depth-dependent properties: Love waves

    - Constructive interference in a low-velocity layer- Dispersion curves- Phase and Group velocity

    Free Oscillations

    - Spherical Harmonics- Modes of the Earth- Rotational Splitting

    Surface waves in an elastic half spaces: Rayleigh waves

    - Potentials- Free surface boundary conditions

    - Solutions propagating along the surface, decaying with depth- Lambs problem

    Surface waves in media with depth-dependent properties: Love waves

    - Constructive interference in a low-velocity layer- Dispersion curves- Phase and Group velocity

    Free Oscillations

    - Spherical Harmonics- Modes of the Earth- Rotational Splitting

    Surface Waves and Free OscillationsSurface Waves and Free Oscillations

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    The Wave Equation: PotentialsThe Wave Equation: Potentials

    Do solutions to the wave equation exist for an elastic half space, whichtravel along the interface? Let us start by looking at potentials:

    i

    i

    zyx

    i

    u

    u

    =

    +=

    ),,(

    scalar potential

    vector potential

    displacement

    These potentials are solutions to the wave equation

    iit

    t

    =

    =

    222

    222

    P-wave speed

    Shear wave speed

    What particular geometry do we want to consider?

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Surface waves: GeometrySurface waves: Geometry

    We are looking for plane waves traveling along one horizontalcoordinate axis, so we can - for example - set

    0(.)=y

    And consider only wave motion in the x,z plane. Then

    As we only require y weset y= from now on. Our

    trial solution is thus

    yxzz

    yzxx

    u

    u

    +=

    =

    )](exp[ xazctikA =

    z

    y

    x

    Wavefront

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Surface waves: Disperion relationSurface waves: Disperion relation

    With this trial solution we obtain for example coefficientsa for which travelling solutions exist

    12

    2

    =

    ca

    Together we obtain

    In order for a plane wave of that form to decay with depth a has to beimaginary, in other words

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    Surface waves: Boundary ConditionsSurface waves: Boundary Conditions

    Analogous to the problem of finding the reflection-transmission coefficients we now have to satisfy theboundary conditions at the free surface (stress free)

    0== zzxz In isotropic media we have

    )]1/(exp[

    )]1/(exp[

    22

    22

    xzcctikB

    xzcctikA

    =

    =

    and

    yxzz

    yzxx

    uu

    +=

    =

    zxxz

    zzzzxxzz

    uuuu

    =

    ++=

    22)( where

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    DisplacementDisplacement

    Putting this value back into our solutionswe finally obtain the displacement in thex-z plane for a plane harmonic surfacewave propagating along direction x

    )(cos)4679.18475.0(

    )(sin)5773.0(

    3933.08475.0

    3933.08475.0

    xctkeeCu

    xctkeeCu

    kzkz

    z

    kzkz

    x

    +=

    =

    This development was first made by Lord Rayleigh in 1885. Itdemonstrates that YES there are solutions to the wave

    equation propagating along a free surface!

    Some remarkable facts can be drawn from this particular form:

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    Lambs ProblemLambs Problem

    -the two components are out of phase by

    for small values of z a particle describes an

    ellipse and the motion is retrograde- at some depth z the motion is linear in z

    - below that depth the motion is again ellipticalbut prograde

    - the phase velocity is independent of k: thereis no dispersion for a homogeneous half space

    - the problem of a vertical point force at thesurface of a half space is called Lambs

    problem (after Horace Lamb, 1904).

    - Right Figure: radial and vertical motion for asource at the surface

    theoretical

    experimental

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    Particle Motion (1)Particle Motion (1)

    How does the particle motion look like?

    theoretical experimental

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    Data ExampleData Example

    theoretical experimental

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    Data ExampleData Example

    Question:

    We derived that Rayleigh waves are non-dispersive!But in the observed seismograms we clearly see ahighly dispersed surface wave train?

    We also see dispersive wave motion on bothhorizontal components!

    Do SH-type surface waves exist?Why are the observed waves dispersive?

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    Love Waves: GeometryLove Waves: Geometry

    In an elastic half-space no SH type surface waves exist. Why?Because there is total reflection and no interaction betweenan evanescent P wave and a phase shifted SV wave as in thecase of Rayleigh waves. What happens if we have layer over a

    half space (Love, 1911) ?

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    Love Waves: TrappingLove Waves: Trapping

    Repeated reflection in a layer over a half space.

    Interference between incident, reflected and transmitted SH waves.

    When the layer velocity is smaller than the halfspace velocity, then thereis a critical angle beyon which SH reverberations will be totally trapped.

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Love Waves: TrappingLove Waves: Trapping

    The formal derivation is very similar to the derivation of the Rayleighwaves. The conditions to be fulfilled are:

    1. Free surface condition

    2. Continuity of stress on the boundary3. Continuity of displacement on the boundary

    Similary we obtain a condition for which solutions exist. This time weobtain a frequency-dependent solution a dispersion relation

    22

    11

    2

    2

    2

    222

    1

    /1/1

    /1/1)/1/1tan(

    c

    ccH

    =

    ... indicating that there are only solutions if ...

    2

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Love Waves: SolutionsLove Waves: Solutions

    Graphical solution ofthe previous equation.Intersection of dashed

    and solid lines yielddiscrete modes.

    Is it possible, now, to

    explain the observeddispersive behaviour?

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Love Waves: modesLove Waves: modes

    Some modes for Love waves

    d h l bW d h l b

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Waves around the globeWaves around the globe

    D E lD t E l

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Data ExampleData Example

    Surface waves travelling around the globe

    Li id l h lfLi id l h lf

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Liquid layer over a half spaceLiquid layer over a half space

    Similar derivation for Rayleigh type motion leads to dispersive behavior

    A lit d A liA lit d A li

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Amplitude AnomaliesAmplitude Anomalies

    What are the effects on the amplitude of surface waves?

    Away from source or antipode geometrical spreading is approx. prop. to (sin)1/2

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    VelocityVelocity

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    VelocityVelocity

    Interference of two waves at two positions (2)

    DispersionDispersion

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    DispersionDispersion

    The typical dispersive behavior of surface wavessolid group velocities; dashed phase velocities

    Wave PacketsWave Packets

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Wave PacketsWave Packets

    Seismograms of a Lovewave train filtered withdifferent central periods.

    Each narrowband tracehas the appearance of awave packet arriving atdifferent times.

    Wave PacketsWave Packets

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Wave PacketsWave Packets

    Group and phasevelocity measurementspeak-and-troughmethod

    Phase velocities fromarray measurement

    DispersionDispersion

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    DispersionDispersion

    Stronger gradients cause greater dispersion

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    Love wave dispersionLove wave dispersion

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Love wave dispersionLove wave dispersion

    Love wave dispersionLove wave dispersion

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Love wave dispersionLove wave dispersion

    Love wave dispersionLove wave dispersion

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Love wave dispersionLove wave dispersion

    Modal SummationModal Summation

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Mo a Summat onmm

    Free oscillations - DataFree oscillations - Data

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    20-hour long recording of agravimeter recordind thestrong earthquake near

    Mexico City in 1985 (tides

    removed). Spikes correspondto Rayleigh waves.

    Spectra of the seismogramgiven above. Spikes atdiscrete frequencies

    correspond toeigenfrequencies of the Earth

    Eigenmodes of a stringEigenmodes of a string

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    g gg g

    Geometry of a string underntension with fixed end points.Motions of the string excited

    by any source comprise aweighted sum of theeigenfunctions (which?).

    Eigenmodes of a sphereEigenmodes of a sphere

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    g pg p

    Eigenmodes of a homogeneoussphere. Note that there are modeswith only volumetric changes (like P

    waves, called spheroidal) and modeswith pure shear motion (like shear

    waves, called toroidal).

    - pure radial modes involve no nodal

    patterns on the surface- overtones have nodal surfaces atdepth

    - toroidal modes involve purelyhorizontal twisting

    - toroidal overtones have nodalsurfaces at constant radii.

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    Bessel and LegendreBessel and Legendre

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Solutions to the wave equation on spherical coordinates: Bessel functions (left)and Legendre polynomials (right).

    Spherical HarmonicsSpherical Harmonics

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Examples of spherical surface harmonics. There are zonal,sectoral and tesseral harmonics.

    The Earths EigenfrequenciesThe Earths Eigenfrequencies

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Spheroidal modeeigenfrequencies

    Toroidal mode

    eigenfrequencies

    Effects of Earths RotationEffects of Earths Rotation

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    non-polar latitude

    polar latitude

    Effects of Earths Rotation: seismogramsEffects of Earths Rotation: seismograms

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    observed

    synthetic no splitting

    synthetic

    Lateral heterogeneityLateral heterogeneity

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Illustration of the distortion of standing-waves

    due to heterogeneity. The spatial shift of thephase perturbs the observed multiplet amplitude

    ExamplesExamples

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Sumatra M9, 26-12-04Sumatra M9, 26-12-04

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Surface Waves: SummarySurface Waves: Summary

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    Seismolo and the Earths Dee Interior Surface Waves and Free Oscillations

    Rayleigh waves are solutions to the elastic wave equation given

    a half space and a free surface. Their amplitude decaysexponentially with depth. The particle motion is elliptical andconsists of motion in the plane through source and receiver.

    SH-type surface waves do not exist in a half space. However

    in layered media, particularly if there is a low-velocitysurface layer, so-called Love waves exist which aredispersive, propagate along the surface. Their amplitude alsodecays exponentially with depth.

    Free oscillations are standing waves which form after bigearthquakes inside the Earth. Spheroidal and toroidaleigenmodes correspond are analogous concepts to P and shearwaves.

    Rayleigh waves are solutions to the elastic wave equation givena half space and a free surface. Their amplitude decaysexponentially with depth. The particle motion is elliptical andconsists of motion in the plane through source and receiver.

    SH-type surface waves do not exist in a half space. Howeverin layered media, particularly if there is a low-velocitysurface layer, so-called Love waves exist which aredispersive, propagate along the surface. Their amplitude alsodecays exponentially with depth.

    Free oscillations are standing waves which form after bigearthquakes inside the Earth. Spheroidal and toroidaleigenmodes correspond are analogous concepts to P and shearwaves.