Diffuse echo bursts at 34.5 MHz

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/205

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DC Field	Value	Language
dc.contributor.author	Subramanian, K. R	-
dc.date.accessioned	2005-01-08T08:39:46Z	-
dc.date.available	2005-01-08T08:39:46Z	-
dc.date.issued	1988	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9. pp. 217-222	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/205	-
dc.description.abstract	The solar radio bursts during their propagation towards the earth are refracted, scattered, reflected and absorbed. The combination of these effects play a role in determining the source size, position, brightness temperature and time profile of solar bursts at the earth. The sporadic radio emission of the sun in some cases reveal features which are called “echo like”. These echo bursts occur during periods of decameter storms. Abranin et al (1982, 1984) first reported these diffuse echo bursts at 25 MHz. We present here further observations on these bursts at a frequency of 34.5 MHz.	-
dc.format.extent	114488 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar radio bursts	en
dc.title	Diffuse echo bursts at 34.5 MHz	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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