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)''
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<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>
 +
 +
<li> '''PMI Focus Group Report''' from the 2008 GEM Meeting:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM2008-PMI_FGReport.doc"
 +
 
<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>
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<li> Jerry Goldstein's notes from all sessions:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/pmi_summary-JGoldstein.doc"
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<li> Mick Denton's notes from the PMI 2 Session:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/pmi_summary-MDenton.doc"
 +
</ol>
 +
 
<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"
 +
 
<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"].)  
<li> '''PMI Focus Group Report''' from the 2008 GEM Meeting:  "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM2008-PMI_FGReport.doc"
+
 
<li>  Miscellaneous '''Notes from PMI Sessions''': 
+
 
<ul>
 
<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"
 
</ul>
 
 
</ul>
 
</ul>
  
<h2>TOPIC:  ''<U>WAVE-PARTICLE INTERACTIONS</U>&nbsp; &nbsp; &nbsp; &nbsp; ''</h2>   
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<h2>TOPIC (I):  ''<U>WAVE-PARTICLE INTERACTIONS</U>&nbsp; &nbsp; &nbsp; &nbsp; ''</h2>   
 
<ul>
 
<ul>
<li>&nbsp; &nbsp; &nbsp; &nbsp;  I. &nbsp; &nbsp; &nbsp; &nbsp; How does the evolving global distribution of cold plasma govern the growth and propagation of waves, specifically those that control energetic particle distributions & dynamics?
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<li>&nbsp; &nbsp; &nbsp; &nbsp;  A. &nbsp; &nbsp; &nbsp; &nbsp; 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> &nbsp; &nbsp; &nbsp; &nbsp; II. &nbsp; &nbsp; &nbsp; &nbsp; How do ambient plasma properties such as temperature, density, and composition influence wave particle interactions?
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<li> &nbsp; &nbsp; &nbsp; &nbsp; B. &nbsp; &nbsp; &nbsp; &nbsp; How do ambient plasma properties such as temperature, density, and composition influence wave particle interactions?
 
</ul>
 
</ul>
  
<h2>TOPIC:  ''<U>PLUME DYNAMICS & RECIRCULATION</U>&nbsp; &nbsp; &nbsp; &nbsp; ''</h2>   
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<h2>TOPIC (II):  ''<U>PLUME DYNAMICS & RECIRCULATION</U>&nbsp; &nbsp; &nbsp; &nbsp; ''</h2>   
 
<ul>
 
<ul>
<li>&nbsp; &nbsp; &nbsp; &nbsp; I. &nbsp; &nbsp; &nbsp; &nbsp; How is eroded plasmaspheric material transported throughout the magnetosphere, and how does it evolve?
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<li>&nbsp; &nbsp; &nbsp; &nbsp; A. &nbsp; &nbsp; &nbsp; &nbsp; How is eroded plasmaspheric material transported throughout the magnetosphere, and how does it evolve?
<li>&nbsp; &nbsp; &nbsp; &nbsp; II.&nbsp; &nbsp; &nbsp; &nbsp; How do plumes influence the reconnection process, and what are the implications for solar-wind-magnetosphere coupling?
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<li>&nbsp; &nbsp; &nbsp; &nbsp; B.&nbsp; &nbsp; &nbsp; &nbsp; 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

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)
Join The GEM PMI E-Mail List: Just send e-mail to Jerry Goldstein.


GEM 2008-2009 Activities & Documents

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?