Differences between revisions 2 and 7 (spanning 5 versions)
Revision 2 as of 2008-02-28 07:06:24
Size: 581
Editor: l4-m0
Comment:
Revision 7 as of 2008-03-20 05:38:54
Size: 682
Editor: sunwave
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:

 * Large-scale and global MHD dynamics - J.Toomre (15 min)
 * Solar Magnetism and Dynamo - J. Stenflo (15 min)
 * Emerging Flux and Sunspots - V. Martinez Pillet (15 min)
 * Links to coronal activity; flare and CME initiation - G. Fisher (15 min)
 * Solar shape and irradiance sources - J. Kuhn (15 min)
 * General discussion (15 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)
 * Characterization of pre-flare magnetic structures and flows - H. Wang (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)
  • {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)
  • Characterization of pre-flare magnetic structures and flows - H. Wang (15 min)


  • Back to [:SDOTeamsMeeting:SDO Teams Meeting Agenda ]

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