Current-less solar wind driven dust acoustic instability in cometary plasma

Physics – Plasma Physics

Scientific paper

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Scientific paper

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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