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- W2045562124 abstract "[1] The whistler anisotropy instability is driven by an electron temperature anisotropy T⊥/T∥ > 1 where ⊥ and ∥ denote directions perpendicular and parallel, respectively, to the background magnetic field Bo. Here kinetic linear theory in a magnetized, homogeneous, collisionless plasma model is used to study this instability when the electron velocity distribution may be represented as the sum of a hot, anisotropic bi-Maxwellian and a cold, isotropic component. The critical β∥e, the value at which the maximum growth rate of the instability changes from propagation parallel to Bo to oblique propagation, decreases with increasing nc/ne, where nc is the cold electron density and ne is the total electron density. At parallel propagation the maximum growth rate increases with nc/ne up to nc/ne ≃ 0.8, but then diminishes with further increases of the relative cold electron density. Introduction of a cold electron component can reduce the hot electron anisotropy necessary to excite this instability by up to a factor of 2." @default.
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- W2045562124 date "2012-07-01" @default.
- W2045562124 modified "2023-10-16" @default.
- W2045562124 title "Whistler anisotropy instability with a cold electron component: Linear theory" @default.
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- W2045562124 doi "https://doi.org/10.1029/2012ja017631" @default.
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