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Detailed Reference Information |
Nishimura, K., Gary, S.P. and Li, H. (2002). Whistler anisotropy instability: Wave-particle scattering rate. Journal of Geophysical Research 107: doi: 10.1029/2002JA009250. issn: 0148-0227. |
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An electron temperature anisotropy T⊥e > T∥e (where ⊥ and ∥ refer to directions relative to the background magnetic field) can excite the whistler anisotropy instability in a collisionless plasma. The resulting enhanced fluctuating magnetic fields scatter the electrons and reduce the anisotropy. We use particle-in-cell simulations in a spatially homogeneous plasma model to compute the maximum values of the wave-particle scattering rate for electron anisotropy reduction. This rate scales as the electron cyclotron frequency but, for a fixed initial growth rate, is relatively independent of the electron temperature if kBTe ≤ 5 keV. For larger electron temperatures, the scattering rate decreases with increasing Te, suggesting that relativistic effects play a role. |
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Abstract |
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Keywords
Magnetospheric Physics, Plasma waves and instabilities, Interplanetary Physics, Plasma waves and turbulence, Space Plasma Physics, Wave/particle interactions, Space Plasma Physics, Numerical simulation studies |
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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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