Low frequency plasma turbulence excited by cometary ions

dc.contributor.author	Lakhina, G.S.
dc.date.accessioned	2015-06-02T05:14:41Z
dc.date.accessioned	2021-02-12T10:28:31Z
dc.date.available	2015-06-02T05:14:41Z
dc.date.available	2021-02-12T10:28:31Z
dc.date.issued	1988
dc.identifier.citation	Plasma theory and nonlinear and turbulent processes in physics, v.2 ed.by V.G.Bar'yakhtar et.al.: Singapore, World Scientific, p.683-689, 1988.	en_US
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/140
dc.description.abstract	Properties of the hydromagnetic turbulence observed near comet Halley are explained by a model consisting of a gas of Alfven solitons generated via the modulational instability of large amplitude Alfven waves excited by picked up cometary ions. The lower hybrid instability excited by the cometary ions' distribution can explain the 0 - 300 Hz electrostatic noise observed near comet Halley.	en_US
dc.language.iso	en	en_US
dc.subject	Hydromagnetic	en_US
dc.subject	Alfven waves	en_US
dc.subject	Cometary ions	en_US
dc.subject	Plasma turbulence	en_US
dc.title	Low frequency plasma turbulence excited by cometary ions	en_US
dc.type	Article	en_US
dc.identifier.accession	090657