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

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<br> Joe Borovsky ''(Plume Dynamics & Recirculation)''
 
<br> Joe Borovsky ''(Plume Dynamics & Recirculation)''
 
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<h3>TOPIC:  ''<U>WAVE-PARTICLE INTERACTIONS</U>&nbsp; &nbsp; &nbsp; &nbsp; ''</h3> 
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<ul>
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<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; II. &nbsp; &nbsp; &nbsp; &nbsp; How do ambient plasma properties such as temperature, density, and composition influence wave particle interactions?
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</ul>
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<h3>TOPIC:  ''<U>PLUME DYNAMICS & RECIRCULATION</U>&nbsp; &nbsp; &nbsp; &nbsp; ''</h3> 
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<ul>
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<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; 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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</ul>

Revision as of 11:24, 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)

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?