Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/363
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dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2005-02-11T02:18:15Z-
dc.date.available2005-02-11T02:18:15Z-
dc.date.issued1986-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 6, pp. 72-76en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/363-
dc.description.abstractThe Continuum emission from the Quiet Sun and active regions is the radiation from the solar atmosphere when there is no transient burst activity. At decametric wavelengths this radiation originates in the outer corona. A study of this radiation offers, therefore, a method of obtaining the density and temperature structure of the outer corona. In this review we provide an account of the observations with the Decameter Wave Radio Telescope at Gauribidanur, and possible interpretation of the origin and variations of the radiation.en
dc.format.extent170375 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectRadio Emissionen
dc.subjectQuiet Sunen
dc.subjectRadio Telescopeen
dc.titleRadio Emission From The Quiet Sun and Active Regions at Decametric Wavelengthsen
dc.typeArticleen
Appears in Collections:Kodaikanal Observatory Bulletins (1905 - 1997 )
IIAP Publications

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