FG11. Plasmasphere-Magnetosphere Interactions
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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)
GEM 2008-2009 Activities & Documents
- PMI Science Questions from the 2008 GEM Meeting: "http://enarc.space.swri.edu/PAPERS/FTP/PMI/PMI-ScienceQuestions.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"].)
- PMI Focus Group Report from the 2008 GEM Meeting: "http://enarc.space.swri.edu/PAPERS/FTP/PMI/GEM2008-PMI_FGReport.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"
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?
