Diff for "ParSess13"

Differences between revisions 2 and 14 (spanning 12 versions)

Helioseismology 1: HMI Initial Science Goals and Targets

-  ⇤ ← Revision 2 as of 2008-02-28 07:06:24 → 
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+   ← Revision 14 as of 2013-05-01 04:35:24 → ⇥
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-=== Tuesday @ 2:30 p.m. ===
+=== Tuesday @ 1:30 p.m. ===
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- * 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)
+ * [[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_1_welsch.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)
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-Back to [:SDOTeamsMeeting:SDO Teams Meeting Agenda ]
+ . Back to [[SDOTeamsMeeting|SDO Teams Meeting Agenda ]]