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Kinetic effects near the magnetopause

Conference ·
OSTI ID:10139101
;  [1];  [2];  [3];  [4];  [5]
  1. Los Alamos National Lab., NM (United States)
  2. California Univ., San Diego, La Jolla, CA (United States)
  3. Lockheed Palo Alto Research Labs., CA (United States)
  4. Dartmouth Coll., Hanover, NH (United States)
  5. John Hopkins Univ., Laurel, MD (United States). Applied Physics Lab.
Boundary conditions for magnetopause processes such as reconnection can be understood by studying the properties of magnetosheath plasma as it flows toward this transition. This manuscript reviews the role of electromagnetic ion cyclotron instabilities in constraining ion temperature anisotropies in the magnetosheath. Linear Vlasov theory and hybrid computer simulations have demonstrated that the inverse correlation between the proton anisotropy and the parallel proton {beta} observed from AMPTE/CCE in the subsolar sheath is due to wave-particle scattering by ion cyclotron anisotropy instabilities. Recent research on this topic is reviewed and the application of this inverse correlation to a successful bounded anisotropy model of proton temperatures in the sheath is described.
Research Organization:
Los Alamos National Lab., NM (United States)
Sponsoring Organization:
USDOE, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States)
DOE Contract Number:
W-7405-ENG-36
OSTI ID:
10139101
Report Number(s):
LA-UR--94-1057; CONF-940393--1; ON: DE94009333
Country of Publication:
United States
Language:
English

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