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

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