Diff for "ParSess13"

Differences between revisions 6 and 12 (spanning 6 versions)

Helioseismology 1: HMI Initial Science Goals and Targets

[: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?:] - Brian Welsch (15 min)
Solar shape and irradiance sources - Jeff Kuhn (15 min)
[attachment:Haimin%5FWang%5Fsdo.ppt Characterization of pre-flare magnetic structures and flows] - H. Wang (15 min)

-  ⇤ ← Revision 6 as of 2008-03-20 05:19:15 → 
  Size: 679
  Editor: sunwave
  Comment:
+   ← Revision 12 as of 2008-03-26 06:58:41 → ⇥
  Size: 796
  Editor: 72-254-55-167
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
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- * 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)
+ * [: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?:] - Brian Welsch (15 min)
 Line 10:
- * H. Wang, Characterization of pre-flare magnetic structures and flows (15 min)
+ * [attachment:Haimin%5FWang%5Fsdo.ppt Characterization of pre-flare magnetic structures and flows] - H. Wang (15 min)
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- Back to [:SDOTeamsMeeting:SDO Teams Meeting Agenda ]
+ . Back to [:SDOTeamsMeeting:SDO Teams Meeting Agenda ]