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

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