Radio Observations of Compact Sources in the Outer Solar Corona

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/252

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.contributor.author	Subramanian, K. R	-
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2005-01-28T06:01:58Z	-
dc.date.available	2005-01-28T06:01:58Z	-
dc.date.issued	1997	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 143-145	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/252	-
dc.description.abstract	We have observed radio emission from the solar corona at a frequency of 77 MHz during the total solar eclipse on October 24, 1995 from our observatory at Gauribidanur. Sources of angular sizes less than or equal to 1.5' have been found to exist at height 0.4Ro above the photosphere.	en
dc.format.extent	64178 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar eclipse	en
dc.subject	Radio emission	en
dc.subject	Scattering	en
dc.title	Radio Observations of Compact Sources in the Outer Solar Corona	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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