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Geol 600 Notable Historical Earthquakes Finite fault rupture propagation rohan.sdsu.edu/~kbolsen/geol600_nhe_source_inversion.ppt.

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Presentation on theme: "Geol 600 Notable Historical Earthquakes Finite fault rupture propagation rohan.sdsu.edu/~kbolsen/geol600_nhe_source_inversion.ppt."— Presentation transcript:

1 Geol 600 Notable Historical Earthquakes Finite fault rupture propagation http://www- rohan.sdsu.edu/~kbolsen/geol600_nhe_source_inversion.ppt

2 9 Force Couples M ij (the moment tensor), 6 different (M ij =M ji ). |M|=fd M 11 M 12 M 13 Good approximation for distant M= M 21 M 22 M 23 earthquakes due to a point source M 31 M 32 M 33 Larger earthquakes can be modeled as sum of point sources

3  Description of earthquakes using moment tensors: Parameters: strike , dip , rake Right-lateral =180 o, left-lateral =0 o, =90 reverse, =-90 normal faulting Strike, dip, rake, slip define the focal mechanism

4  Description of earthquakes using moment tensors: M 11 = -M 0 (sin  cos sin2  s + sin2  sin sin 2  s ), M 12 = M 0 (sin  cos cos2  s + 0.5 sin2  sin sin2  s ), M 13 = -M 0 (cos  cos cos  s + cos2  sin sin  s ), M 22 = M 0 (sin  cos sin2  s - sin2  sin cos 2  s ), M 23 = -M 0 (cos  cos sin  s - cos2  sin cos  s ), M 33 = M 0 sin2  sin 

5 P-waves S-waves

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8 Finite-size Fault Plane Divide into ‘sub-faults’ ‘sub-faults’ x x x x

9 Define rupture parameters (distributions of slip, rake, rupture speed, source-time function, stress, friction, etc) wave-propagation code Compute synthetic seismograms at receiver locations Compare synthetic to observed seismograms Synthetics fit data? Yes no

10 Kinematic source inversion: Solves for slip history on the fault Dynamic source inversion: Solves for stress and friction on the fault

11 Kinematic Source Inversion

12 Landers: Classic Vertical Strike-Slip Event

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14 Test case: 1992 M 7.3 Landers Well-recorded event

15 Slip-weakening Rupture Model

16 Dynamic Rupture From Trial-and-Error Finite-Difference Modeling

17 How is rupture propagation affected by realistic variation of dynamic parameters? Let’s look at changes in the stress drop…

18 Inverted (Trial-and- Error) Dynamic Radiation Versus Data

19 Stress Field (a)

20 Stress Field (b)

21 Stress Field (c)

22 1994 M6.7 Northridge

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24 2004 M6.0 Parkfield

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26 1999 M7.4 Izmit

27 SOURCE TIME FUNCTION DURATION ALSO VARIES WITH STATION AZIMUTH FROM FAULT. THIS DIRECTIVITY CAN CONSTRAIN WHICH NODAL PLANE IS THE FAULT PLANE For earthquake, V/V R ~1.2 for shear waves and 2.2 for P waves. Maximum duration is 180° from the rupture direction, and the minimum is in the rupture direction. Analogous effect: thunder generated by sudden heating of air along a lightning channel in the atmosphere. Here V/V R ~0, so observers perpendicular to the channel hear a brief, loud, thunder clap, whereas observers in the channel direction hear a prolonged rumble. Directivity similar to Doppler Shift, but differs in requiring finite source dimension Stein & Wysession, 2003


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