Actions for Ion Bernstein instability in the magnetosphere [electronic resource] : linear dispersion theory

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Ion Bernstein instability in the magnetosphere [electronic resource] : linear dispersion theory

Published
Washington, D.C. : United States. Dept. of Energy, 2010.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Additional Creators
Los Alamos National Laboratory, United States. Department of Energy, and United States. Department of Energy. Office of Scientific and Technical Information
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Summary
Nonthermal ion velocity distributions may drive kinetic instabilities which lead to enhanced field fluctuations near ω{sub r} ≈ Ω{sub p} in the magnetosphere. These fluctuations resonate with, and thus scatter, both ions and electrons. Ions are thermalized. Fast electrons undergo both pitch-angle scattering and acceleration.
Report Numbers
E 1.99:la-ur-10-08230
E 1.99: la-ur-10-8230
la-ur-10-8230
la-ur-10-08230
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Note
Published through SciTech Connect.
12/10/2010.
"la-ur-10-08230"
" la-ur-10-8230"
2010 Fall AGU Meeting ; December 13, 2010 ; San Francisco, CA.
Liu, Kaijun; Winske, Dan; Gary, S Peter.
Funding Information
AC52-06NA25396
View MARC record | catkey: 13804322