Dust acoustic instability driven by solar and stellar winds

dc.contributor.author	Vranjes, J.
dc.date	2011
dc.date.accessioned	2016-03-29T12:43:54Z
dc.date.available	2016-03-29T12:43:54Z
dc.identifier.uri	https://orfeo.belnet.be/handle/internal/3146
dc.description	A quantitative analysis is presented of the dust acoustic wave instability driven by the solar or stelar wind. This is a current-less kinetic instability which develops in permeating plasmas, i.e., when one quasi-neutral electron-ion plasma propagates through another quasi-neutral plasma which contains dust, electrons and ions. The cometary dusty plasma in the solar wind appears to be practically always unstable.
dc.language	eng
dc.title	Dust acoustic instability driven by solar and stellar winds
dc.type	Conference
dc.subject.frascati	Physical sciences
dc.audience	Scientific
dc.source.title	AIP Conference Proceedings
dc.source.volume	1397
dc.source.page	407-408
Orfeo.peerreviewed	No
dc.identifier.doi	10.1063/1.3659866
dc.identifier.scopus	2-s2.0-84255201084