Difference between revisions of "FG11. Plasmasphere-Magnetosphere Interactions"
		
		
		
		
		
		
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<br>'''Topic Chairs:'''  Maria Spasojevic  ''(Wave-Particle Interactions)''  | <br>'''Topic Chairs:'''  Maria Spasojevic  ''(Wave-Particle Interactions)''  | ||
<br> Joe Borovsky ''(Plume Dynamics & Recirculation)''  | <br> Joe Borovsky ''(Plume Dynamics & Recirculation)''  | ||
| + | <br> <font color="green"><b>Join The GEM PMI E-Mail List:</b>  </font>Just send e-mail to Jerry Goldstein.  | ||
<div align=left>  | <div align=left>  | ||
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<h2>GEM 2008-2009 Activities & Documents</h2>  | <h2>GEM 2008-2009 Activities & Documents</h2>  | ||
<ul>  | <ul>  | ||
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| + | <li> '''PMI Focus Group Report''' from the 2008 GEM Meeting:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM2008-PMI_FGReport.doc"  | ||
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<li> PMI '''Science Questions''' from the 2008 GEM Meeting:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/PMI-ScienceQuestions.doc"  | <li> PMI '''Science Questions''' from the 2008 GEM Meeting:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/PMI-ScienceQuestions.doc"  | ||
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| + | <li>  Miscellaneous '''Notes from PMI Sessions''':    | ||
| + | <ol>  | ||
| + | <li> Jerry Goldstein's notes from all sessions:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/pmi_summary-JGoldstein.doc"  | ||
| + | <li> Mick Denton's notes from the PMI 2 Session:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/pmi_summary-MDenton.doc"  | ||
| + | </ol>  | ||
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<li> '''PMI Sessions''' at the 2008 GEM Meeting:   "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM-PMI-08.xls"  | <li> '''PMI Sessions''' at the 2008 GEM Meeting:   "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM-PMI-08.xls"  | ||
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<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"  | ||
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<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> <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"].)    | ||
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</ul>  | </ul>  | ||
| − | <h2>TOPIC:  ''<U>WAVE-PARTICLE INTERACTIONS</U>        ''</h2>     | + | <h2>TOPIC (I):  ''<U>WAVE-PARTICLE INTERACTIONS</U>        ''</h2>     | 
<ul>  | <ul>  | ||
| − | <li>           | + | <li>         A.	        How does the evolving global distribution of cold plasma govern the growth and propagation of waves, specifically those that control energetic particle distributions & dynamics?  | 
| − | <li>           | + | <li>         B.	        How do ambient plasma properties such as temperature, density, and composition influence wave particle interactions?  | 
</ul>  | </ul>  | ||
| − | <h2>TOPIC:  ''<U>PLUME DYNAMICS & RECIRCULATION</U>        ''</h2>     | + | <h2>TOPIC (II):  ''<U>PLUME DYNAMICS & RECIRCULATION</U>        ''</h2>     | 
<ul>  | <ul>  | ||
| − | <li>          | + | <li>        A.	        How is eroded plasmaspheric material transported throughout the magnetosphere, and how does it evolve?  | 
| − | <li>          | + | <li>        B.        How do plumes influence the reconnection process, and what are the implications for solar-wind-magnetosphere coupling?  | 
</ul>  | </ul>  | ||
Revision as of 12:50, 2 July 2008
Contents
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)
 Join The GEM PMI E-Mail List:  Just send e-mail to Jerry Goldstein.
GEM 2008-2009 Activities & Documents
- PMI Focus Group Report from the 2008 GEM Meeting: "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM2008-PMI_FGReport.doc"
 - PMI Science Questions from the 2008 GEM Meeting: "http://enarc.space.swri.edu/PAPERS/FTP/PMI/PMI-ScienceQuestions.doc"
 -   Miscellaneous Notes from PMI Sessions:  
- Jerry Goldstein's notes from all sessions: "http://enarc.space.swri.edu/PAPERS/FTP/PMI/pmi_summary-JGoldstein.doc"
 - Mick Denton's notes from the PMI 2 Session: "http://enarc.space.swri.edu/PAPERS/FTP/PMI/pmi_summary-MDenton.doc"
 
 - PMI Sessions at the 2008 GEM Meeting: "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM-PMI-08.xls"
 - Original Focus Group Proposal: "http://enarc.space.swri.edu/PAPERS/FTP/PMI/PMI-FG-Proposal_v2.doc"
 - Want to Join the GEM PMI E-Mail List? 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). (Note from JG: 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"].)
 
TOPIC (I): WAVE-PARTICLE INTERACTIONS
- A. How does the evolving global distribution of cold plasma govern the growth and propagation of waves, specifically those that control energetic particle distributions & dynamics?
 - B. How do ambient plasma properties such as temperature, density, and composition influence wave particle interactions?
 
TOPIC (II): PLUME DYNAMICS & RECIRCULATION
- A. How is eroded plasmaspheric material transported throughout the magnetosphere, and how does it evolve?
 - B. How do plumes influence the reconnection process, and what are the implications for solar-wind-magnetosphere coupling?
 
