Difference between revisions of "GEM Focus Groups"
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# [[FG10. Diffuse Auroral Precipitation|Diffuse Auroral Precipitation]] (2006 - 2011, RA: [[RA-MIC|MIC]], [[RA-IMS|IMS]]) | # [[FG10. Diffuse Auroral Precipitation|Diffuse Auroral Precipitation]] (2006 - 2011, RA: [[RA-MIC|MIC]], [[RA-IMS|IMS]]) | ||
# [[FG11. Plasmasphere-Magnetosphere Interactions|Plasmasphere-Magnetosphere Interactions]] (2008 - 2013, RA: [[RA-IMS|IMS]]) | # [[FG11. Plasmasphere-Magnetosphere Interactions|Plasmasphere-Magnetosphere Interactions]] (2008 - 2013, RA: [[RA-IMS|IMS]]) | ||
− | # [[FG12. Substorm Expansion Onset|Substorm Expansion Onset]] (2008 - 2013, RA: [[RA-Tail|Tail]]) | + | # [[FG12. Substorm Expansion Onset: The First 10 Minutes|Substorm Expansion Onset: The First 10 Minutes]] (2008 - 2013, RA: [[RA-Tail|Tail]]) |
# [[FG13. Modes of Solar WInd-Magnetosphere Energy Transfer|Modes of Solar WInd-Magnetosphere Energy Transfer]] (2008 - 2013, RA: [[RA-Tail|Tail]]) | # [[FG13. Modes of Solar WInd-Magnetosphere Energy Transfer|Modes of Solar WInd-Magnetosphere Energy Transfer]] (2008 - 2013, RA: [[RA-Tail|Tail]]) | ||
Revision as of 14:14, 16 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)
- 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: 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