Difference between revisions of "GEM Focus Groups"
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# [[FG3. Foreshock, Bowshock, Magnetosheath|Foreshock, Bowshock, Magnetosheath]] (2004 - 2009, RA: [[RA-Dayside|Dayside]]) | # [[FG3. Foreshock, Bowshock, Magnetosheath|Foreshock, Bowshock, Magnetosheath]] (2004 - 2009, RA: [[RA-Dayside|Dayside]]) | ||
# [[FG4. Plasma Entry and Transport into and within the Magnetotail|Plasma Entry and Transport into and within the Magnetotail]] (2006 - 2011, RA: [[RA-Tail|Tail]]) | # [[FG4. Plasma Entry and Transport into and within the Magnetotail|Plasma Entry and Transport into and within the Magnetotail]] (2006 - 2011, RA: [[RA-Tail|Tail]]) | ||
| − | # [[FG5. | + | # [[FG5. Dayside Magnetopause Reconnection|Dayside Magnetopause Reconnection]] (2004 - 2009, RA: [[RA-Dayside|Dayside]]) |
# [[FG6. Cusp Physics|Cusp Physics]] (2006-2010, RA: [[RA-Dayside|Dayside]]) | # [[FG6. Cusp Physics|Cusp Physics]] (2006-2010, RA: [[RA-Dayside|Dayside]]) | ||
# [[FG7. MIC Electrodynamics|MIC Electrodynamics]] (2003 - 2008, RA: [[RA-MIC|MIC]]) | # [[FG7. MIC Electrodynamics|MIC Electrodynamics]] (2003 - 2008, RA: [[RA-MIC|MIC]]) | ||
Revision as of 11:22, 25 September 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)
- 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)
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
