The frequency drift and time splitting of decameter solar radio bursts

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4415

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2009-03-25T10:48:01Z	-
dc.date.available	2009-03-25T10:48:01Z	-
dc.date.issued	1972-05	-
dc.identifier.citation	Astrophysical Letters, Vol. 11, pp. 47 - 51	en
dc.identifier.issn	0888-6512	-
dc.identifier.uri	http://hdl.handle.net/2248/4415	-
dc.description.abstract	The frequency drift and time splitting of solar radio bursts are observed with a multi-channel radiometer and a polarimeter at frequencies around 25 MHz. It is found that a majority of noise storm bursts have drift rates between + 1.0 and -1.0 MHz/sec. Two types of unusual bursts with frequency drift are described. The two components of a double burst are found to be polarized to the same degree and in the same sense.	-
dc.language.iso	en	en
dc.publisher	Gordon and Breach, Science Publishers Ltd.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1972ApL....11...47S	en
dc.subject	Frequency Drift	en
dc.subject	Time Splitting of Decameter	en
dc.subject	Solar Radio Bursts	en
dc.title	The frequency drift and time splitting of decameter solar radio bursts	en
dc.type	Article	en
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