Difference between revisions of "FG11. Plasmasphere-Magnetosphere Interactions"

From gem
Jump to navigation Jump to search
Line 13: Line 13:
 
<li> PMI Sessions At 2008 GEM Meeting:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM-PMI-08.xls"
 
<li> PMI Sessions At 2008 GEM Meeting:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM-PMI-08.xls"
 
<li> Original Focus Group Proposal:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/PMI-FG-Proposal_v2.doc"
 
<li> Original Focus Group Proposal:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/PMI-FG-Proposal_v2.doc"
 +
<li> <font color="green"><b>Want to Join the GEM PMI E-Mail List?</b>  </font>Just send e-mail to Jerry Goldstein with your (1)  Name, (2)  E-mail address, and (3) What you will be doing during the coming year (#3 is optional, but useful for planning).  (<b><i><u>Note from JG</u></i></b>:  My e-mail is not posted here, to protect against spammers.  My e-mail string can be constructed as:  [first initial] + [last name] + ["at" symbol] + [my affiliation, SwRI] + ["dot edu"].)
 +
<li>
 
</ul>
 
</ul>
  

Revision as of 14:16, 1 July 2008

PMI-Logo2-sm-land.jpg

Plasmasphere-Magnetosphere Interactions (PMI)

How Are Magnetospheric Processes Regulated By Plasmaspheric Dynamics (and Vice Versa)?

Conveners: Jerry Goldstein, Joe Borovsky
Topic Chairs: Maria Spasojevic (Wave-Particle Interactions)
Joe Borovsky (Plume Dynamics & Recirculation)

GEM 2008-2009 Activities & Documents

TOPIC: WAVE-PARTICLE INTERACTIONS       

  •         I.         How does the evolving global distribution of cold plasma govern the growth and propagation of waves, specifically those that control energetic particle distributions & dynamics?
  •         II.         How do ambient plasma properties such as temperature, density, and composition influence wave particle interactions?

TOPIC: PLUME DYNAMICS & RECIRCULATION       

  •         I.         How is eroded plasmaspheric material transported throughout the magnetosphere, and how does it evolve?
  •         II.        How do plumes influence the reconnection process, and what are the implications for solar-wind-magnetosphere coupling?