Low frequency solar radio astronomy at the Indian Institute of Astrophysics (IIA)

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5699

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.date.accessioned	2012-02-17T11:07:03Z	-
dc.date.available	2012-02-17T11:07:03Z	-
dc.date.issued	2011	-
dc.identifier.citation	ASI Conference Series, Vol. 2, pp. 55-61	en
dc.identifier.isbn	978-81-922926-0-1	-
dc.identifier.uri	http://hdl.handle.net/2248/5699	-
dc.description	Open Access	en
dc.description.abstract	IIA is presently involved in the expansion of its existing radioheliograph operating in the frequency 120-40 MHz at the Gauribidanur radio observatory located about 80 km north of Bangalore. Once completed, the expanded array will have an angular resolution of ~1` at a typical frequency of 100 MHz. This paper describes the development of solar radio astronomy activities at IIA since 1952 when the first observations were carried out.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.rights	© Astronomical Society of India	en
dc.subject	Sun: corona	en
dc.subject	Sun: radio radiation – telescopes	en
dc.title	Low frequency solar radio astronomy at the Indian Institute of Astrophysics (IIA)	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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