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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/395
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dc.contributor.authorGopalswamy, N-
dc.contributor.authorThejappa, G-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2005-05-14T09:30:04Z-
dc.date.available2005-05-14T09:30:04Z-
dc.date.issued1984-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 4, pp. 47-54en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/395-
dc.description.abstractThe Solar decametric radio emission consists of a variety of fine structures. This reflects the complexity of the corona at this level. Two observations, viz. absorption bursts and short duration narrow band bursts are presented. An interpretation of each of these observations is provided.en
dc.format.extent359341 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectSolar Coronaen
dc.subjectRadio Burstsen
dc.titleObservations on the Fine Structures in Solar Decametric Radio Emissionen
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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