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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4111
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dc.contributor.authorKrishan, V-
dc.date.accessioned2008-12-18T14:14:59Z-
dc.date.available2008-12-18T14:14:59Z-
dc.date.issued1980-12-
dc.identifier.citationSolar Physics, Vol. 68, No. 2, pp. 343 - 350en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/4111-
dc.description.abstractAn energetic proton beam passing through a stationary ionized medium, excites ion-acoustic turbulence. The ion-acoustic instability saturates due to the non-linear indirect wave-particle scattering. The electric field associated with the ion-acoustic waves accelerates the plasma particles. Applicability of the results to cometary tails is discussed.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1980SoPh...68..343Ken
dc.relation.urihttp://dx.doi.org/10.1007/BF00156873en
dc.subjectIon Acoustic Wavesen
dc.subjectMagnetohydrodynamic Stabilityen
dc.subjectPlasma Accelerationen
dc.subjectPlasma Turbulenceen
dc.subjectPlasma Wavesen
dc.subjectSolar Winden
dc.subjectComet Tailsen
dc.subjectLinear Equationsen
dc.subjectPlasma-Particle Interactionsen
dc.subjectProton Beamsen
dc.subjectSpace Plasmasen
dc.titlePlasma acceleration by ion-acoustic turbulenceen
dc.typeArticleen
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