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    U.S. Department of the Interior 

    U.S. Geological Survey

    Earthquake Focal Mechanisms

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    Focal Mechanism Solutions

     Also called “ beachball diagrams” “ fault planesolutions”

    Tell us the geometry and mechanism of thefault in a simple diagram

    Generally reconstructed from waveform data

    derived from the moment tensor (which ismore general), but originally calculated using

    first motions – done here to illustrate the

    concepts

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    Examples

    USGS

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    1) The stereographic projection

    2) The geometry of first motions and how this is

    used to define fault motion.

    Two steps to understanding

    http://www.uwsp.edu/geo/projects/geoweb/participants/dutch/STRUCTGE/sphproj.htm

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    Stereographic projection

     A method of projectinghalf a sphere onto a circle.

    e.g. planes cuttingvertically through the

    sphere plot as straight

    lines

    Images from http://www.learninggeoscience.net/free/00071/index.html

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    Stereonets

     A template

    called a

    stereonet

    is used to

    plot data.

    Example –

    plottingplanes

    (e.g. faults)

    USGS

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    Stereonets

    Example –

    plottinglines (e.g.

    ray paths)

    USGS

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    Stereonets

    Example –pitch (or

    rake) of a line

    on a plane(e.g. the slip

    direction on a

    fault)

    USGS

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    Refresher on terminology

    USGS

    Slip angle is measured from horizontal

    (positive for thrusts)

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    Energy and Polarity of “ First Motions”

    Cox and Hart. Plate Tectonics – How it works.

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    Earthquake on a vertical plane

    Edited from Cox and Hart. Plate Tectonics – How it works.

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    Determination of nodal planes

    Cox and Hart. Plate Tectonics – How it works.

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    Spreading of the seismic wave

    Cox and Hart. Plate Tectonics – How it works.

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    Data on thesurface,

    interpreted in3D

    Cox and Hart. Plate Tectonics – How it works.

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    Take-off angle

    The angle (from vertical) that the ray leavesthe earthquake = take-off angle

    Stein and Wysession, An Introduction to seismology, earthquakes and Earth structure

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     Azimuth ( ) andtake-off angle

    USGS

    Stein and Wysession, An Introduction to seismology, earthquakes and Earth structure

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    With a lot of recordings we can

    reconstruct faults with any orientations

    Cox and Hart. Plate Tectonics – How it works.

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    Fault types and “ Beach Ball” plots

    USGS

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    Example Focal

    mechanismdiagrams on mid-

    ocean ridges

    Stein and Wysession, An Introduction to seismology, earthquakes and Earth structure

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    Same N-S fault,

    different slip direction

    Stein and Wysession, An Introduction to seismology, earthquakes and Earth structure

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    Great review on the web at:

    http://www.learninggeoscience.net/free/00071/

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    By constructing

    synthetic seismograms

    and comparing them tothe recorded data we

    use more of the

    information in the

    seismogram, not just

    the arrival time and firstmotion data

    Waveform modeling

    Stein and Wysession, “An Introduction to

    seismology, earthquakes and Earth structure”

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    Waveform modeling

    u(t) = x(t) * e(t) * q(t) * i(t) 

    seismogram

    source timefunction instrument

    responsereflections &

    conversionsat interfaces

    attenuation

    U( ω  )= X( ω  ) E( ω  ) Q( ω  ) I( ω  ) 

    Construction

    of the

    syntheticseismogram

    Stein and Wysession, “An Introduction to seismology,

    earthquakes and Earth structure”

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     At one point on the fault slip takes a finitetime (called “ rise time” ):

    The slip travels along the fault at rupture

    velocity vr, so there is also a finite “ rupture

    time”

    Source-time function

    Time

       S   l   i  p

    TDTime

       S   l   i  p  r  a   t  e

    TD

    Time

       S   l   i  p

      r  a   t  e

    TR

    Fault= rupture

    Map view

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    Source time function

    The source time function is the combinationof the rise time and the rupture time:

    Directionality affects the rupture time

    Time   S   l   i  p

      r  a   t  e

    TDTime

       S   l   i  p

      r  a   t  e

    TR

       S   l   i  p

      r  a   t  e

    TR TD* =

    TR TD

    TR TD

    TR TD

    TR TDRupture direction

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    phase reflections

    e(t) representsreflections due to

    the Earth

    structure

    If modeling only

    the P arrival, it’sonly needed for

    shallow events

    Stein and Wysession, “An Introduction to seismology, earthquakes and Earth structure”

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     Attenuation

    The loss of energy with time

    Q controls the

    amount of loss

     A(t) = A 0 

     

    e - ω 0 t/2Q 

    Sipkin and Jordan 1979, copywrite

    Seismological Society of America

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    Instrument response function

    The response of the seismometer is different

    for different frequencies so it also filters thedata.

    Stein and Wysession, “An Introduction to seismology,

    earthquakes and Earth structure”

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    Moment Tensor Inversion

    The Moment tensor describes the fault as setof equivalent forces

    Calculated from the amplitude of surfacewaves Love Rayleigh

    USGS