GEM Focus Groups
		
		
		
		
		
		
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- 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)
 - Component versus Anti-parallel 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 (2008 - 2013, RA: Tail)
 - Modes of Solar WInd-Magnetosphere Energy Transfer (2008 - 2013, RA: Tail)
 
(RA: Research Area)
Joint GEM-SHINE Sessions
- 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