Radio spectrograph observations of the recent soalr eclipse on October 24, 1995

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/253

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DC Field	Value	Language
dc.contributor.author	Shanmugaraju, A	-
dc.contributor.author	Umapathy, S	-
dc.date.accessioned	2005-01-28T06:11:39Z	-
dc.date.available	2005-01-28T06:11:39Z	-
dc.date.issued	1997	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 147-149	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/253	-
dc.description.abstract	A solar radio spectrograph has been developed to observe the transient solar radio emissions in the band of 30 MHz at our School of Physics. A non trackable log periodic antenna having beam of 60 degree in E-W and 90 degree in N-S is being used. The recent solar eclipse of October 24, 1995 was observed with maximum obstruction of sun's disc by moon to the tune of 40% using the above radio spectrograph. The initial results have been reported in this paper.	en
dc.format.extent	65574 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Banglaore	en
dc.subject	Solar eclipse	en
dc.subject	Radio spectrograph	en
dc.title	Radio spectrograph observations of the recent soalr eclipse on October 24, 1995	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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