Observations on the occultation of the radio source Tauras A by the solar corona during June 1971

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4674

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch. V	-
dc.contributor.author	Subramanian, K. R	-
dc.date.accessioned	2009-07-24T11:09:59Z	-
dc.date.available	2009-07-24T11:09:59Z	-
dc.date.issued	1974-09	-
dc.identifier.citation	Indian Journal of Radio and Space Physics, Vol. 4, pp. 196 - 198	en
dc.identifier.issn	0367-8393	-
dc.identifier.uri	http://hdl.handle.net/2248/4674	-
dc.description.abstract	Observations on the occultation of the radio source Tamas A (3C 144) during June 1971 at a wavelength of 12 m are presented. It is tentatively observed that there is no strong dependence between the amount of scattering and solar activity.	en
dc.language.iso	en	en
dc.publisher	National Institute of Science Communication and Information Resources	en
dc.subject	Radio Source Tauras	en
dc.subject	Solar Corona	en
dc.subject	Occultation	en
dc.title	Observations on the occultation of the radio source Tauras A by the solar corona during June 1971	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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