Differences between revisions 1 and 5 (spanning 4 versions)
Revision 1 as of 2008-01-23 05:17:54
Size: 202
Editor: l4-m0
Comment:
Revision 5 as of 2008-03-15 04:30:06
Size: 637
Editor: l4-m0
Comment:
Deletions are marked like this. Additions are marked like this.
Line 1: Line 1:
=== Tuesday p.m. 1 === === Tuesday @ 1:30 p.m. ===
Line 3: Line 3:
== Local HS 1: SDO/HMI Issues == == Helioseismology 1: HMI Initial Science Goals and Targets ==
Line 7: Line 7:
Local HS 1: SDO/HMI Issues === Agenda (90 min) ===
Line 9: Line 9:
 * 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)
 * {i} [: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)
 * General discussion (15 min)
----

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)
  • {i} [: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)
  • General discussion (15 min)


Back to [:SDOTeamsMeeting:SDO Teams Meeting Agenda ]

JsocWiki: ParSess13 (last edited 2013-05-01 04:35:24 by localhost)