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Observations and interpretation of solar decametric absorption bursts

dc.contributor.authorGopalswamy, N.
dc.contributor.authorThejappa, N.
dc.contributor.authorSastry, Ch.V.
dc.date.accessioned2006-01-03T04:47:24Z
dc.date.available2006-01-03T04:47:24Z
dc.date.issued1983
dc.description.abstractThe observations of intensity reductions or absorption bursts in the solar decametric radio-continuum are reported. The reductions are interpreted as the absorption of continuum radiation by a shock-generated ion sound turbulence present in the layer above the continuum level. The duration of the absorption is attributed to the life-time of the ion-sound turbulence while the depth of absorption is determined by the level of Langmuir waves generated as a result of absorption.en
dc.format.extent1018567 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationJournal of Astrophysics and Astronomy, 1983, Vol. 4, p215-224.en
dc.identifier.issn0250-6335
dc.identifier.urihttp://hdl.handle.net/2289/1053
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.subjectSunen
dc.subjectDecametric absurption burstsen
dc.subjectIon-sound turbulenceen
dc.titleObservations and interpretation of solar decametric absorption burstsen
dc.typeArticleen

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