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| ===== Leaders: Deborah Haber & Tom Duvall (1) Bob Stein & Konstantin Parchevsky (2) ===== | ===== Leaders: Deborah Haber & Tom Duvall (Part 1), Bob Stein & Konstantin Parchevsky (Part 2) ===== |
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| . What data are already available. . What is being planned to be done. |
. What data are already available? . What is being planned to be done? |
Tuesday @ 3:30 p.m.
Local HS 2: Techniques & Comparisons, Simulations & Validations
Leaders: Deborah Haber & Tom Duvall (Part 1), Bob Stein & Konstantin Parchevsky (Part 2)
Part 1: Techniques and Intercomparison (45 minutes)
1. Systematic errors, Deborah Haber
2. Random error estimates - time-distance, Sebastien Couvidat
3. MDI ring diagram frequency variations, Rachel Howe)
4. Comparison of ring diagram and tine-distance results, Brad Hindman
5. Comparison of MDI, GONG with HMI, Tom Duvall
Part 2: Numerical Simulations and Validation of Local Helioseismology (45 minutes)
1. Realistic Non linear simulations
Supergranulation Scale Solar Surface Convection Simulations, (8 min) Dali Georgobiani
Realistic numerical simulations of solar magneto-convection, (8 min) Laetitia Jacoutot
2. Linear Wave Modeling
Far Side Modeling (TBC), (8 min) Thomas Hartlep
MHD simulations (TBC), (8 min) Shravan Hanasoge
3. General Discussion, Konstantin Parchevski
- What data are already available?
- What is being planned to be done?
- List of standard tests.
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