Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/208

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2005-01-08T08:52:02Z	-
dc.date.available	2005-01-08T08:52:02Z	-
dc.date.issued	1988	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 227	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/208	-
dc.description.abstract	The brightness temperature distribution of the quiet solar corona at a wavelength of 8.9 Meters is measured with two types of radio telescopes: (1) A “ T ” type array with a resolution of 26’x38’ and (2) A fan beam interferometer with an E-W resolution of 3’. It is found that the persistent bright regions do not have any angular structure on scales 6’ or less. The daily variations of the brightness temperature of different regions are studied and the possible interpretation in discussed.	-
dc.format.extent	11965 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar Corona	en
dc.title	Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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