Difference between revisions of "M8 PSHA Analysis"

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#Given event has a one year probability as  0.000020546511 or annual occurrence probability of 1 in 48,670.066
 
#Given event has a one year probability as  0.000020546511 or annual occurrence probability of 1 in 48,670.066
  
[[File:UCERF2_M8.jpg|256px|thumb|right|Fig 1: SCEC Intern development SCEC-VDO displaying a UCERF2.0 rupture representative of the M8 rupture. SCEC-VDO animates the CyberShake SRF files showing hypocenter and rupture velocity.]]
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[[File:UCERF2_M8.jpg|256px|thumb|left|Fig 1: SCEC Intern development SCEC-VDO displaying a UCERF2.0 rupture representative of the M8 rupture. SCEC-VDO animates the CyberShake SRF files showing hypocenter and rupture velocity.]]
  
 
== M8 PSHA Peak Ground Motion Map ==
 
== M8 PSHA Peak Ground Motion Map ==
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[[Image:sa1.0-shakemap-89-03.png|256px|thumb|right|Fig 2: Peak Spectral Acceleration at 1Hz for the UCERF2.0 M8-equivalent rupture.]]
 
[[Image:sa1.0-shakemap-89-03.png|256px|thumb|right|Fig 2: Peak Spectral Acceleration at 1Hz for the UCERF2.0 M8-equivalent rupture.]]
  
 
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[[Image:sa1.0-cb2008-89-03.png|256px|thumb|left|Fig 3: Peak Spectral Acceleration at 1Hz for the UCERF2.0 M8-equivalent rupture using Campbell and Bozorgnia attenuation Relationship.]]
[[Image:sa1.0-shakemap-89-03.png|256px|thumb|right|Fig 2: Peak Spectral Acceleration at 1Hz for the UCERF2.0 M8-equivalent rupture using ShakeMap attenuation relationship.]]
 
 
 
 
 
[[Image:sa1.0-cb2008-89-03.png|256px|thumb|right|Fig 3: Peak Spectral Acceleration at 1Hz for the UCERF2.0 M8-equivalent rupture using Campbell and Bezorgnia attenuation Relationiship.]]
 
  
 
[[Image:gmrotD50_01.00Hz.bin.png|256px|thumb|right|Fig 4 M8 map showing Peak Spectral Acceleration at 1Hz using wave propagation.]]
 
[[Image:gmrotD50_01.00Hz.bin.png|256px|thumb|right|Fig 4 M8 map showing Peak Spectral Acceleration at 1Hz using wave propagation.]]

Revision as of 19:48, 7 October 2010

The M8 PSHA analysis compares estimated ground motions for M8 using standard empirical attenuation relationship methods versus full wave propagation results. The UCERF2 also provide probabilities for this event using current best estimates.

UCERF2 M8 Rupture Match:

The UCERF 2.0 rupture from CyberShake that matches M8 was found using the following guidelines:

  1. Use SCEC-VDO SRF Plugin to access a list of UCERF2.0 ruptures with 1 year probabilities.
  2. Select CyberShake Ruptures ID:35 (Rupture Set 34 has been deprecated)
  3. Select Source that includes the San Andreas Segments included in the M8 fault. We have selected Source ID 89 as the source that includes San Andreas Segments PK,CH,CC, BB, NM,SM,NSB,SSB,BG, and C0.
  4. Select Rupture Variation Scenario ID: 3. Scenario ID 4 is new as of the SCEC Annual meeting 2010 and has not been used in any CyberShake calculations.
  5. Select a Rupture ID with Magnitude similar to M8. We select Rupture ID 3 with M8.05 and Probability: 2.0546511e-5
  6. Select a rupture variation with a hypocenter location near the M8 hypocenter (-120.396396, 35.846868, -16,000).
  7. Selected event is 89_3 variation S0055-H0026 with Hypocenter at (-120.3858, 35.849, -15.5655) as closest matching UCERF rupture.
  8. Given event has a one year probability as 0.000020546511 or annual occurrence probability of 1 in 48,670.066
Fig 1: SCEC Intern development SCEC-VDO displaying a UCERF2.0 rupture representative of the M8 rupture. SCEC-VDO animates the CyberShake SRF files showing hypocenter and rupture velocity.

M8 PSHA Peak Ground Motion Map

Fig 2: Peak Spectral Acceleration at 1Hz for the UCERF2.0 M8-equivalent rupture.
Fig 3: Peak Spectral Acceleration at 1Hz for the UCERF2.0 M8-equivalent rupture using Campbell and Bozorgnia attenuation Relationship.
Fig 4 M8 map showing Peak Spectral Acceleration at 1Hz using wave propagation.


M8 CyberShake Peak Ground Motion Map