High Angular Resolution Radio Observations of the Outer Solar Corona

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3157

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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	2008-08-18T06:52:15Z	-
dc.date.available	2008-08-18T06:52:15Z	-
dc.date.issued	2000	-
dc.identifier.citation	Advances in Space Research, Vol. 25, No. 9, pp. 1847 - 1850	en
dc.identifier.issn	0273-1177	-
dc.identifier.uri	http://hdl.handle.net/2248/3157	-
dc.description	Restricted Access	en
dc.description.abstract	We report high angular resolution observations of the outer solar corona carried out at 75 MHz from the Gauribidanur Radio Observatory (Long: 77°26'12" E, Lat: 13°36'12" N) about 100 km north of Bangalore, India, during the solar eclipse of October 24, 1995. Our main conclusion is that there are structures of angular size <= 2.5' in the outer solar corona at a height of <<< 0.4 R⊚ above the photosphere	en
dc.format.extent	320635 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Elsevier	en
dc.relation.uri	http://dx.doi.org/doi:10.1016/S0273-1177(99)00596-7	en
dc.subject	High angular resolution	en
dc.subject	Outer solar corona	en
dc.title	High Angular Resolution Radio Observations of the Outer Solar Corona	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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