Low frequency plasma turbulence excited by cometary ions

dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-06-02T05:14:41Z
dc.date.accessioned2021-02-12T10:28:31Z
dc.date.available2015-06-02T05:14:41Z
dc.date.available2021-02-12T10:28:31Z
dc.date.issued1988
dc.description.abstractProperties 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.identifier.accession090657
dc.identifier.citationPlasma 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.urihttp://library.iigm.res.in:4000/handle/123456789/140
dc.language.isoenen_US
dc.subjectHydromagneticen_US
dc.subjectAlfven wavesen_US
dc.subjectCometary ionsen_US
dc.subjectPlasma turbulenceen_US
dc.titleLow frequency plasma turbulence excited by cometary ionsen_US
dc.typeArticleen_US

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