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arXiv 1108.2158physics.plasm-phastro-ph.SR
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Current-less solar wind driven dust acoustic instability in cometary plasma

J. Vranjes

英文摘要:

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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