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• W2031874148 startingPage "135" @default.
• W2031874148 abstract "Auroral electron precipitation in the morning sector is assumed to be the result of an electromagnetic cyclotron instability of a particle distribution that evolves adiabatically as its constituent electrons drift eastward from a source near midnight. The adiabatic distribution is calculated by using Green's function in various magnetospheric field models, and the corresponding growth rates for whistler mode waves are calculated by the method of Kennel and Petschek (1966). The region of maximum calculated wave growth corresponds spatially and temporally to the region of maximum observed electron precipitation only when the magnetospheric electric field is included realistically in the model." @default.
• W2031874148 created "2016-06-24" @default.
• W2031874148 creator A5069536725 @default.
• W2031874148 date "1976-01-01" @default.
• W2031874148 modified "2023-09-26" @default.
• W2031874148 title "Electron precipitation in the morning sector of the auroral zone" @default.
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• W2031874148 doi "https://doi.org/10.1029/ja081i001p00135" @default.
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