GEM Focus Groups: Difference between revisions

Revision as of 08:19, 11 August 2009

GGCM Metrics and Validation (2005 - 2010, RA: GGCM)
GGCM Modules and Methods (2005 - 2010, RA: GGCM)
Foreshock, Bowshock, Magnetosheath (2004 - 2009, RA: Dayside)
Plasma Entry and Transport into and within the Magnetotail (2006 - 2011, RA: Tail)
Dayside Magnetopause Reconnection (2004 - 2009, RA: Dayside)
Cusp Physics (2006-2010, RA: Dayside)
MIC Electrodynamics (2003 - 2008, RA: MIC)
Near Earth Magnetosphere: plasma, fields, and coupling (2007 - 2012, RA: IMS, Tail)
Space Radiation Climatology (2006 - 2011, RA: IMS, see also FG9 google email group)
Diffuse Auroral Precipitation (2006 - 2011, RA: MIC, IMS)
Plasmasphere-Magnetosphere Interactions (2008 - 2013, RA: IMS)
Substorm Expansion Onset: The First 10 Minutes (2008 - 2013, RA: Tail)
Modes of Solar WInd-Magnetosphere Energy Transfer (2008 - 2013, RA: Tail)

(RA: Research Area)

@@ Line 16: / Line 16: @@
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-'''Joint GEM-SHINE Sessions'''
+==GEM Planning Activities==
-#[[Solar-Wind Drivers or Internal Magnetospheric Processes]]
-#[[Creation and Propagation of CMEs and Plasmoids: Loss of Equilibrium and Subsequent Evolution]]
-#[[Small-Scale Structure in the Solar Wind and Its Effect on Earth]]
-#[[Is there a Need for More-Detailed Solar-Wind Models]]
-#[[What Determines When Reconnection Turns On? Chromosphere,Corona, Solar Wind, Magnetopause, and Magnetotail]]
-#[[SEPs from Heliosphere to Magnetosphere]]
-#[[Comparing the Properties of Magnetic Reconnection in Various Environments]]
-#[[Perpendicular Ion Heating: Observations at Earth and theory at the Sun]]