Hank Childs, University of Oregon Lecture #2 Fields, Meshes, and Interpolation (Part 1)
Nuclear Energy Work Hank Childs & Christoph Garth April 15, 2010.
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Transcript of Nuclear Energy Work Hank Childs & Christoph Garth April 15, 2010.
Customers, team, & goals
• Customers: Argonne NEAMS personnel, especially INCITE awardee Paul Fischer
• VACET team members: Hank Childs & Christoph Garth– Activity normally leveraged by NEAMS vis $’s
• Goal: ensure visualization and analysis needs continued to be met successfully and analysis aid in advanced analysis.
• Customers: Argonne NEAMS personnel, especially INCITE awardee Paul Fischer
• VACET team members: Hank Childs & Christoph Garth– Activity normally leveraged by NEAMS vis $’s
• Goal: ensure visualization and analysis needs continued to be met successfully and analysis aid in advanced analysis.
This work depends on efficient streamline
generation (described in later talks)We needed parallel efficient
streamline techniques to do this work. (SC09)
We needed parallel efficient streamline techniques to do this
work. (SC09)
Computational Astrophysics Consortium
• Team: Hank Childs, Gunther Weber, Allen Sanderson• Customers:
– Jay Salmonson, LLNL– Christian Ott & Reiswig, CalTech– John Bell & Ann Almgren, LBL (Maestro)– Adam Burrows, Jason Nordhaus & Princeton team (Castro)
• Note: much of this effort is leveraged by NERSC Analytics
• Goal: Ensure CAC visualization and analysis needs are met
• Team: Hank Childs, Gunther Weber, Allen Sanderson• Customers:
– Jay Salmonson, LLNL– Christian Ott & Reiswig, CalTech– John Bell & Ann Almgren, LBL (Maestro)– Adam Burrows, Jason Nordhaus & Princeton team (Castro)
• Note: much of this effort is leveraged by NERSC Analytics
• Goal: Ensure CAC visualization and analysis needs are met
Streamlines with astrophysics data
• Upcoming analysis: use streamlines to study flow through the center of the star and better understand how neutrinos get irradiated.
• Upcoming analysis: use streamlines to study flow through the center of the star and better understand how neutrinos get irradiated.