Radio Emission From The Quiet Sun and Active Regions at Decametric Wavelengths

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/363

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2005-02-11T02:18:15Z	-
dc.date.available	2005-02-11T02:18:15Z	-
dc.date.issued	1986	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 72-76	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/363	-
dc.description.abstract	The 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.extent	170375 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Radio Emission	en
dc.subject	Quiet Sun	en
dc.subject	Radio Telescope	en
dc.title	Radio Emission From The Quiet Sun and Active Regions at Decametric Wavelengths	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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