Differences between revisions 9 and 13 (spanning 4 versions)
Revision 9 as of 2008-03-22 03:57:45
Size: 728
Editor: sunwave
Comment:
Revision 13 as of 2008-03-26 07:17:05
Size: 838
Editor: 72-254-55-167
Comment:
Deletions are marked like this. Additions are marked like this.
Line 7: Line 7:
 * 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)
 * [:ValentinMartinezPillet abstract:Emerging Flux and Sunspots] - Valentin Martinez Pillet (15 min)
 * [:WelschAbstract:What can HMI's helioseismic capabilities tell us about flares & CMEs?] ([attachment:Helioseis%5F%31%5Fwelsch.ppt ppt])- Brian Welsch (15 min)
Line 10: Line 10:
 * Characterization of pre-flare magnetic structures and flows - H. Wang (15 min)  * [attachment:Haimin_Wang_sdo.ppt Characterization of pre-flare magnetic structures and flows] - H. Wang (15 min)

Tuesday @ 1:30 p.m.

Helioseismology 1: HMI Initial Science Goals and Targets

Leaders: Juri Toomre & Sasha Kosovichev

Agenda (90 min)

  • [:JuriToomre abstract:Large-scale and global MHD dynamics] - Juri Toomre (15 min)

  • [:JanStenflo abstract:Solar Magnetism and Dynamo] - Jan Stenflo (15 min)

  • [:ValentinMartinezPillet abstract:Emerging Flux and Sunspots] - Valentin Martinez Pillet (15 min)

  • [:WelschAbstract:What can HMI's helioseismic capabilities tell us about flares & CMEs?] ([attachment:Helioseis%5F%31%5Fwelsch.ppt ppt])- Brian Welsch (15 min)

  • Solar shape and irradiance sources - Jeff Kuhn (15 min)
  • [attachment:Haimin_Wang_sdo.ppt 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)