Current-less solar wind driven dust acoustic instability in cometary plasma
arXiv:1108.2158 · doi:10.1063/1.3619819
Abstract
A quantitative analysis is presented of the dust acoustic wave instability driven by the solar and stellar winds. This is a current-less kinetic instability which develops in permeating plasmas, i.e.., when one quasi-neutral electron-ion wind plasma in its propagation penetrates through another quasi-neutral plasma which contains dust, electrons and ions.
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