Difference between revisions of "GEM Focus Groups"
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m (Changed FG labels to sequential numbers.) |
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(RA: Research Area) | (RA: Research Area) | ||
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+ | ---- | ||
+ | '''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]] |
Revision as of 12:33, 11 July 2008
- 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