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• W1778628052 abstract "[1] Radiation belt diffusion codes require, as inputs, precomputed scattering rates, which are currently bounce-averaged in the dipole magnetic field. We present the results of computations of the bounce-averaged quasi-linear pitch-angle diffusion coefficients of relativistic electrons for various distances and two MLT in the Tsyganenko 89c magnetic field model. The coefficients were computed for quiet and storm-time conditions. We compare scattering rates bounce-averaged in a non-dipole field model with those in the dipole field. We demonstrate that on the day side the effects of taking into account a realistic magnetic field are negligible at distances less than six Earth radii. On the night side diffusion coefficients may significantly depend on the assumed field model. Pitch-angle scattering rates calculated in the non-dipole field can explain the often observed night-side chorus induced precipitation. The physical explanation for the changes of pitch-angle scattering rates with the field model is presented and discussed." @default.
• W1778628052 created "2016-06-24" @default.
• W1778628052 creator A5031387835 @default.
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• W1778628052 date "2010-03-01" @default.
• W1778628052 modified "2023-10-06" @default.
• W1778628052 title "Dependence of pitch-angle scattering rates and loss timescales on the magnetic field model" @default.
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• W1778628052 doi "https://doi.org/10.1029/2009gl041639" @default.
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