ShakeMovies - Revision history

Maechlin: /* Examples of SCEC Earthquake Animations */

2022-11-11T06:57:02Z

Examples of SCEC Earthquake Animations

Maechlin: /* Examples of SCEC Earthquake Animations */

2022-11-11T06:54:31Z

Examples of SCEC Earthquake Animations

Maechlin: /* Examples of SCEC Earthquake Animations */

2022-11-11T06:47:51Z

Examples of SCEC Earthquake Animations

Maechlin: /* Examples of SCEC Earthquake Animations */

2022-11-11T06:46:54Z

Examples of SCEC Earthquake Animations

Maechlin at 06:45, 11 November 2022

2022-11-11T06:45:27Z

Maechlin at 09:08, 6 September 2019

2019-09-06T09:08:21Z

Maechlin at 09:04, 6 September 2019

2019-09-06T09:04:36Z

Maechlin at 09:02, 6 September 2019

2019-09-06T09:02:27Z

Maechlin at 08:58, 6 September 2019

2019-09-06T08:58:28Z

Maechlin: /* Examples of SCEC Earthquake Animations */

2019-09-06T08:56:19Z

Examples of SCEC Earthquake Animations

@@ Line 48: / Line 48: @@
 | EQ_Northridge_Site_Pacoima - Simulation showing the effects of ground motions on objects in Pacoima, about 12km from epicenter of Northridge Earthquake. The animation was created by retrieving the observed ground motions from a Pacoima strong motion station for the Northridge earthquake, then inputting these seismograms into a scene containing everyday objects, and using a physics-engine to show the results of the ground motions on the objects.
 |-
-| [[File:vmag_side_by_side.png|150px|thumb|left| Fig 11: TeraShake Rupture Directivity Comparison (Image Credit: Amit Chourasia Steve Cutchin (SDSC)]]
+| [[File:vmag_side_by_side.png|150px|thumb|left| Fig 11: TeraShake Rupture Directivity Comparison (Image Credit: Amit Chourasia, Steve Cutchin, Marcio Faerman (SDSC)]]
 | [https://youtu.be/iYhnN63xToI Animation_11]
 | Comparison of Velocity Magnitudes For TeraShake Ruptures - This animation compares two equivalent TeraShake Ruptures on the San Andreas Fault. Both ruptures are identical except for the slip direction. This animation shows multiple variables in an understandable way including location and magnitude of the instantaneous peak velocity in both ruptures, the distribution and magnitude of peak ground motions for both ruptures, and the rupture and wave propagation time and duration.

@@ Line 49: / Line 49: @@
 |-
 | [[File:vmag_side_by_side.png|150px|thumb|left| Fig 11: TeraShake Rupture Directivity Comparison (Image Credit: Amit Chourasia Steve Cutchin (SDSC)]]
-| [https://youtu.be/sUTqTlkGUws Animation_11]
+| [https://youtu.be/iYhnN63xToI Animation_11]
 | Comparison of Velocity Magnitudes For TeraShake Ruptures - This animation compares two equivalent TeraShake Ruptures on the San Andreas Fault. Both ruptures are identical except for the slip direction. This animation shows multiple variables in an understandable way including location and magnitude of the instantaneous peak velocity in both ruptures, the distribution and magnitude of peak ground motions for both ruptures, and the rupture and wave propagation time and duration.
 |-

@@ Line 48: / Line 48: @@
 | EQ_Northridge_Site_Pacoima - Simulation showing the effects of ground motions on objects in Pacoima, about 12km from epicenter of Northridge Earthquake. The animation was created by retrieving the observed ground motions from a Pacoima strong motion station for the Northridge earthquake, then inputting these seismograms into a scene containing everyday objects, and using a physics-engine to show the results of the ground motions on the objects.
 |-
-| [[File:vmag_side_by_side.png|150px|thumb|left| Fig 11: TeraShake Rupture Directivity Comparison (Image Credit: Amit Chourasia Steve Cutchin (SDSC))) ]]
+| [[File:vmag_side_by_side.png|150px|thumb|left| Fig 11: TeraShake Rupture Directivity Comparison (Image Credit: Amit Chourasia Steve Cutchin (SDSC)]]
-| [https://youtu.be/sUTqTlkGUws Animation_10]
+| [https://youtu.be/sUTqTlkGUws Animation_11]
-| Comparison of Velocity Magnitudes For TeraShake Ruptures - This animation compares two equivalent TeraShake Ruptures on the San Andreas Fault. Both ruptures are identical except for the slip direction. This animation shows multiple variables in an understandable way including location and magnitude of instantaneous peak velocity in both ruptures, the distribution and magnitude of peak ground motions for both ruptures, and the rupture and wave propagation time and duration.
+| Comparison of Velocity Magnitudes For TeraShake Ruptures - This animation compares two equivalent TeraShake Ruptures on the San Andreas Fault. Both ruptures are identical except for the slip direction. This animation shows multiple variables in an understandable way including location and magnitude of the instantaneous peak velocity in both ruptures, the distribution and magnitude of peak ground motions for both ruptures, and the rupture and wave propagation time and duration.
 |-
 | [[File:BSZ Many Models.png|150px|thumb|left| Fig 12: Brawley Seismic Zone Dynamic Rupture (Image Credit: Christos Kyriakopoulos)(Univ of Memphis/CERI)) ]]
-| [http://hypocenter.usc.edu/research/BSZ_CK/videos/Many_Models.mp4 Animation_11]
+| [http://hypocenter.usc.edu/research/BSZ_CK/videos/Many_Models.mp4 Animation_12]
 | This video shows four different dynamic rupture models, all based on a postulated network of faults in the Salton Sea area, southern California. The hypocenter of these events is placed on the San Andreas fault and approximately 30km north of Bombay beach. The first seconds of the simulations show the initiation phase of the earthquake, also known as the “nucleation phase”. After this initial phase, the earthquake rupture propagates spontaneously towards the right-hand side of the screen (south-east in the map). More information can be found on [[Brawley Seismic Zone Simulations]].
 |}

@@ Line 50: / Line 50: @@
 | [[File:vmag_side_by_side.png|150px|thumb|left| Fig 11: TeraShake Rupture Directivity Comparison (Image Credit: Amit Chourasia Steve Cutchin (SDSC))) ]]
 | [https://youtu.be/sUTqTlkGUws Animation_10]
-| Comparison of Velocity Magnitudes For TeraShake Ruptures - This animation compares two equivalent TeraShake Ruptures on the San Andreas Fault. Both ruptures are identical except for the slip direction. This comparison animations shows multiple variables in an understandable way including location and magnitude of instantaneous peak velocity in both ruptures, the distribution and magnitude of peak ground motions for both ruptures, and the rupture and wave propagation time and duration.
+| Comparison of Velocity Magnitudes For TeraShake Ruptures - This animation compares two equivalent TeraShake Ruptures on the San Andreas Fault. Both ruptures are identical except for the slip direction. This animation shows multiple variables in an understandable way including location and magnitude of instantaneous peak velocity in both ruptures, the distribution and magnitude of peak ground motions for both ruptures, and the rupture and wave propagation time and duration.
 |-
 | [[File:BSZ Many Models.png|150px|thumb|left| Fig 12: Brawley Seismic Zone Dynamic Rupture (Image Credit: Christos Kyriakopoulos)(Univ of Memphis/CERI)) ]]

@@ Line 48: / Line 48: @@
 | EQ_Northridge_Site_Pacoima - Simulation showing the effects of ground motions on objects in Pacoima, about 12km from epicenter of Northridge Earthquake. The animation was created by retrieving the observed ground motions from a Pacoima strong motion station for the Northridge earthquake, then inputting these seismograms into a scene containing everyday objects, and using a physics-engine to show the results of the ground motions on the objects.
 |-
-| [[File:BSZ Many Models.png|150px|thumb|left| Fig 11: Brawley Seismic Zone Dynamic Rupture (Image Credit: Christos Kyriakopoulos)(Univ of Memphis/CERI)) ]]
+| [[File:vmag_side_by_side.png|150px|thumb|left| Fig 11: TeraShake Rupture Directivity Comparison (Image Credit: Amit Chourasia Steve Cutchin (SDSC))) ]]
 | [http://hypocenter.usc.edu/research/BSZ_CK/videos/Many_Models.mp4 Animation_11]
 | This video shows four different dynamic rupture models, all based on a postulated network of faults in the Salton Sea area, southern California. The hypocenter of these events is placed on the San Andreas fault and approximately 30km north of Bombay beach. The first seconds of the simulations show the initiation phase of the earthquake, also known as the “nucleation phase”. After this initial phase, the earthquake rupture propagates spontaneously towards the right-hand side of the screen (south-east in the map). More information can be found on [[Brawley Seismic Zone Simulations]].