arXiv · 1108.2158
Current-less solar wind driven dust acoustic instability in cometary plasma
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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J. Vranjes. 2011-08-10. Current-less solar wind driven dust acoustic instability in cometary plasma. https://doi.org/10.1063/1.3619819
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