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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4108
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dc.contributor.authorGopalswamy, N-
dc.contributor.authorThejappa, G-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-12-17T16:48:15Z-
dc.date.available2008-12-17T16:48:15Z-
dc.date.issued1983-09-
dc.identifier.citationJournal of Astrophysics and Astronomy , Vol. 4, pp. 215 - 224en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/4108-
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.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1983JApA....4..215Gen
dc.relation.urihttp://www.springerlink.com/content/56v88406n848x223/en
dc.rights© Indian Academy of Sciencesen
dc.subjectAbsorption Spectraen
dc.subjectDecametric Wavesen
dc.subjectIon Acoustic Wavesen
dc.subjectPlasma Turbulenceen
dc.subjectSolar Radio Burstsen
dc.subjectContinuous Radiationen
dc.subjectElectrostatic Wavesen
dc.subjectMicrostructureen
dc.subjectRadio Telescopesen
dc.titleObservations and interpretation of solar decametric absorption burstsen
dc.typeArticleen
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