Difference between revisions of "CME Meeting 2011"
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== SCEC/CME Meeting Agenda Sept 11, 2011 == | == SCEC/CME Meeting Agenda Sept 11, 2011 == | ||
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| + | [[File:M8-1.0-Vmag-Height-Field (00153).png|256px|thumb|right|Fig 1: Twenty one seconds after origin time for the SCEC M8 simulation showing instantaneous velocity magnitude as exaggerated topography. Image shows formation of a Mach cone at the leading of the M8 rupture as it progresses south at supershear velocity on Southern San Andreas Fault. (Image Credit: Amit Chourasia (SDSC), Yifeng Cui (SDSC), Kim Olsen (SDSU)]] | ||
Meeting Format: Researchers and research groups present their current and planned calculations with a two slide limit and a strict 10 minute limit including presentation and discussion. | Meeting Format: Researchers and research groups present their current and planned calculations with a two slide limit and a strict 10 minute limit including presentation and discussion. | ||
Revision as of 22:59, 9 September 2011
Contents
SCEC/CME Computational Science Planning Meeting 2011
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Fig 1: Twenty one seconds after origin time for the SCEC M8 simulation showing instantaneous velocity magnitude as exaggerated topography. Image shows formation of a Mach cone at the leading of the M8 rupture as it progresses south at supershear velocity on Southern San Andreas Fault. (Image Credit: Amit Chourasia (SDSC), Yifeng Cui (SDSC), Kim Olsen (SDSU)
- Organizers: T. H. Jordan, P. Maechling
- Date: Sunday, September 11, 2011 (1:00pm – 3:30pm)
- Location: Hilton Palm Springs Resort, Palm Springs, CA
- Address: 400 East Tahquitz Canyon Way, Palm Springs, CA,92262-6605
- Room: Oasis Room III (3rd Floor)
SCEC/CME Meeting Agenda Sept 11, 2011
Fig 1: Twenty one seconds after origin time for the SCEC M8 simulation showing instantaneous velocity magnitude as exaggerated topography. Image shows formation of a Mach cone at the leading of the M8 rupture as it progresses south at supershear velocity on Southern San Andreas Fault. (Image Credit: Amit Chourasia (SDSC), Yifeng Cui (SDSC), Kim Olsen (SDSU)
Meeting Format: Researchers and research groups present their current and planned calculations with a two slide limit and a strict 10 minute limit including presentation and discussion.
Session One: 1:00pm - 2:10pm Current Computational Projects
- Ma-FE on Cobalt - Shuo Ma
- SORD at TACC and ALCF - Geoff Ely
- Hanging Wall Problem for NGA-W - Sandarsh Kumar
- Parallel Broadband - Gaurang Mehta/Mats Rynge
- Chino Hills Higher Frequency - Jacobo Bielak
- California SI Inversion - En-Jui Lee/Po Chen
- Broadband CyberShake - Scott Callaghan
- AWP-ODC-SGT and AWP-ODC-GPU - Jun Zhou
- UCERF3 "Grand" Inversion: A Distributed Simulated Annealing Approach - Kevin Milner
Session Two: 2:20pm - 3:30pm: Future Computational Projects
- Earthquake Simulators - James H. Dieterich
- Dynamic Rupture Modeling - Jeremy Kozdon
- UCVM Development - Brad Aagaard
- Impact of small-scale CVM heterogeneity on Ground Motion Sims - Kim Olsen
- CyberShake 3.0 Map - Philip Maechling
- Computational Science Research Opportunities - Yifeng Cui
- NSF Earth Cube - TBD
- NSF Geoinformatics - TBD
SCEC Meeting Times
We recognize that the CME meeting times overlap with related SCEC workshops listed here: [1]. Several CME group members want to participate in both meetings. To support these collaborative meetings, we will keep the CME meeting informal so that CME participants can move freely moving between meetings. We will try to keep the CME meeting on schedule so that you can determine when specific topics will be discussed at the CME meeting.
- VShaker Overview (PDF Poster)
- SCEC/CME Overview (PDF Poster)
- CVM-Toolkit (PDF Poster)
- Broadband Platform (PDF Poster
- CSEP Testing Center (PDF Poster)
- Milner Operational Earthquake Forecasting Poster (PDF Poster)
- Leonardo Ramirez Central US Velocity Model with Hercules (Powerpoint Poster)
