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Pitch-angle scattering rates in planetary magnetospheres

Published online by Cambridge University Press:  10 May 2005

D. SUMMERS
Affiliation:
Department of Mathematics and Statistics, Memorial University of Newfoundland, St. John's, Newfoundland A1C5S7, Canada (dsummers@math.mun.ca) School of Physics, University of KwaZulu-Natal (Howard College campus), Durban 4041, South Africa
R. L. MACE
Affiliation:
School of Physics, University of KwaZulu-Natal (Pietermaritzburg campus), Private Bag X01, Scottsville 3209, South Africa
M. A. HELLBERG
Affiliation:
School of Physics, University of KwaZulu-Natal (Howard College campus), Durban 4041, South Africa

Abstract

The mechanism of gyroresonant scattering of charged particles by small-amplitude, broadband electromagnetic waves is examined. By means of quasi-linear theory, a simple expression for the resonant pitch-angle diffusion coefficient $D_{\alpha \alpha}$ is developed, which is valid for parallel-propagating, small-amplitude, (R-mode or L-mode) electromagnetic waves of general spectral density. We calculate the average diffusion coefficient with respect to the pitch-angle $\alpha$, namely $\langle D_{\alpha\alpha}\rangle$, which provides a practical estimate for particle scattering rates as a function of particle kinetic energy. The results for $\langle D_{\alpha\alpha}\rangle$, corresponding to a Gaussian wave frequency spectrum, are used to estimate scattering rates for several types of wave–particle interactions in the terrestrial and Jovian magnetospheres.

Type
Papers
Copyright
2005 Cambridge University Press

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