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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4867
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dc.contributor.authorGopalswamy, N-
dc.contributor.authorThejappa, G-
dc.date.accessioned2009-10-16T11:10:25Z-
dc.date.available2009-10-16T11:10:25Z-
dc.date.issued1985-11-
dc.identifier.citationPramana, Vol. 25, No. 5, pp. 575 - 585en
dc.identifier.issn0304-4289-
dc.identifier.urihttp://hdl.handle.net/2248/4867-
dc.description.abstractThe dispersion relation for ion sound waves generated in a perpendicular shock is derived and the energy density of ion-sound turbulence is obtained using quasilinear theory. The result is compared with the lower hybrid turbulence generated under similar conditions. It is shown that ion-sound turbulence is a better candidate for the generation of type-I radio bursts in the solar corona.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://www.ias.ac.in/j_archive/pramana/25/vol25contents.htmlen
dc.rights© Indian Academy of Sciencesen
dc.subjectIon-Sound Turbulenceen
dc.subjectQuasilinear Effectsen
dc.subjectLower Hybrid Turbulenceen
dc.subjectType-I Radio Burstsen
dc.titleIon-sound turbulence due to shock gradients in collisionless plasmasen
dc.typeArticleen
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