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- W2588415488 abstract "The evolution of the whistler anisotropy instability relevant to whistler-mode chorus waves in the Earth's inner magnetosphere is studied using kinetic simulations and is compared with satellite observations. The electron distribution is constrained by the whistler anisotropy instability to a marginal stability state and presents an upper bound of electron anisotropy, which agrees with satellite observations. The electron beta β∥e separates whistler waves into two groups: (i) quasi-parallel whistler waves for and (ii) oblique whistler waves close to the resonance cone for . Landau damping is important in the saturation and relaxation stage of the oblique whistler wave growth. The saturated magnetic field energy of whistler waves roughly scales with the electron beta , shown in both simulations and satellite observations. These results suggest the critical role of electron beta β∥e in determining the whistler wave properties in the inner magnetosphere." @default.
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- W2588415488 date "2017-02-01" @default.
- W2588415488 modified "2023-10-13" @default.
- W2588415488 title "On the parameter dependence of the whistler anisotropy instability" @default.
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- W2588415488 doi "https://doi.org/10.1002/2017ja023895" @default.
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