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Detailed Reference Information |
Gary, S.P., Yin, L. and Winske, D. (2000). Electromagnetic proton cyclotron anisotropy instability: Wave-particle scattering rate. Geophysical Research Letters 27: doi: 10.1029/2000GL000055. issn: 0094-8276. |
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The electromagnetic proton cyclotron instability is driven by a proton temperature anisotropy T⊥p/T∥p>1 where the directional subscripts denote directions relative to the background magnetic field. Enhanced field fluctuations from instability growth lead to wave-particle scattering which reduces the anisotropy; previous research has demonstrated that the anisotropy is constrained by a power-law function of &bgr;∥p. Here two-dimensional hybrid simulations in a homogeneous, magnetized, collisionless plasma are used to derive a scaling relation for the maximum scattering rate of proton anisotropy reduction. The result is a function only of the anisotropy and &bgr;∥p and so is appropriate for use in fluid models of anisotropic plasmas such as the magnetosheath. ¿ 2000 American Geophysical Union |
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Abstract |
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Keywords
Magnetospheric Physics, Magnetosheath, Magnetospheric Physics, Magnetotail, Space Plasma Physics, Waves and instabilities |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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