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- W2093515229 abstract "In this paper we develop a model to analyze the electrostatic waves produced in the shock foot at Jupiter. We show that an ion beam instability involving the ions reflected at the shock ramp and the incoming solar wind electrons produces waves at the observed frequencies and that saturation via orbit diffusion limits the waves to amplitudes near to what is observed. Results from two‐dimensional model of the reflected beam in the foot indicates that the waves propagate against the solar wind away from the shock ramp and are amplified up to their saturation amplitudes. The saturation results combined with the electron temperature profile due to wave‐particle interactions predicted by quasi‐linear theory reproduce a wave amplitude profile for the shock foot that is in reasonable agreement with the observations." @default.
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- W2093515229 date "1988-08-01" @default.
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- W2093515229 title "Generation, saturation, and convection of electrostatic waves in Jupiter's shock foot" @default.
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- W2093515229 doi "https://doi.org/10.1029/ja093ia08p08483" @default.
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