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- W2155979307 abstract "The energetic anti-loss-cone electrons can drive a low-frequency electrostatic instability, propagating transverse to the ambient magnetic field, in the presence of a cold plasma. The typical real frequency and growth rates associated with this instabifity are respectively, of the order of (ω p being the proton cyclotron frequency). The instability has a transverse wavelength ⋍10ρ e (ρ e being the Larmor radius of energetic electrons). For the parameters pertinent to auroral plasma at 1R E , the quasi-linear analysis shows that the instability can give rise to an oscillating electric field E sat ⋍0.5−25 mV/ m and an increase of 10 0 –10 3 K in the temperature of cold electrons. The instability may be relevant to recent observations of low-frequency turbulence on the auroral field lines." @default.
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- W2155979307 date "1980-10-01" @default.
- W2155979307 modified "2023-09-26" @default.
- W2155979307 title "Low-frequency electrostatic instability due to anti-loss-cone electrons" @default.
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- W2155979307 doi "https://doi.org/10.1017/s0022377800022789" @default.
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