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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3001
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dc.contributor.authorThejappa, G-
dc.contributor.authorSastry, Ch. V-
dc.contributor.authorGopalswamy, N-
dc.date.accessioned2008-08-05T07:15:18Z-
dc.date.available2008-08-05T07:15:18Z-
dc.date.issued1984-
dc.identifier.citationNonlinear and turbulent processes in physics; Proceedings of the Second International Workshop, Vol. 1, pp. 547 - 561.en
dc.identifier.urihttp://hdl.handle.net/2248/3001-
dc.description.abstractObservations and interpretations of some of the fine structure in decametric solar radio emission -such as (1) the time structure of type III bursts, (2) absorption bursts, and (3) slowly drifting spikes -are presented. Physical parameters -such as the electron temperature, the characteristics of collisionless shocks, and the coronal magnetic field -are estimated.en
dc.format.extent453900 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherHarwood Academic Publishersen
dc.subjectSolar radio emissionen
dc.subjectCoronol magnetic fielden
dc.subjectBurstsen
dc.titleFine structure in solar decametric radiationen
dc.typeArticleen
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