|
Size: 596
Comment:
|
Size: 679
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 1: | Line 1: |
| === Tuesday @ 2:30 p.m. === |
=== Tuesday @ 1:30 p.m. === |
| Line 4: | Line 3: |
| Line 6: | Line 4: |
| Line 8: | Line 5: |
| Line 12: | Line 8: |
| * Links to coronal activity; flare and CME initiation - Brian Welsch (15 min) | * {i} [:WelschAbstract:What can HMI's helioseismic capabilities tell us about flares & CMEs?:] - Brian Welsch (15 min) |
| Line 14: | Line 10: |
| * General discussion (15 min) | * H. Wang, Characterization of pre-flare magnetic structures and flows (15 min) |
| Line 16: | Line 12: |
| Back to [:SDOTeamsMeeting:SDO Teams Meeting Agenda ] | Back to [:SDOTeamsMeeting:SDO Teams Meeting Agenda ] |
Tuesday @ 1:30 p.m.
Helioseismology 1: HMI Initial Science Goals and Targets
Leaders: Juri Toomre & Sasha Kosovichev
Agenda (90 min)
- Large-scale and global MHD dynamics - Juri Toomre (15 min)
- Solar Magnetism and Dynamo - Jan Stenflo (15 min)
- Emerging Flux and Sunspots - Valentin Martinez Pillet (15 min)
[:WelschAbstract:What can HMI's helioseismic capabilities tell us about flares & CMEs?:] - Brian Welsch (15 min) - Solar shape and irradiance sources - Jeff Kuhn (15 min)
- H. Wang, Characterization of pre-flare magnetic structures and flows (15 min)
Back to [:SDOTeamsMeeting:SDO Teams Meeting Agenda ]
