The time splitting of decameter solar radio bursts

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4412

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2009-03-25T10:36:04Z	-
dc.date.available	2009-03-25T10:36:04Z	-
dc.date.issued	1971-03	-
dc.identifier.citation	Astrophysical Letters, Vol. 8, pp. 115 - 119	en
dc.identifier.issn	0888-6512	-
dc.identifier.uri	http://hdl.handle.net/2248/4412	-
dc.description.abstract	Solar radio bursts were observed with a multi-channel receiver with frequency separations of 100 to 200 kHz: at a center frequency of 25 MHz. The time resolution was 15 msec. Some properties of double bursts are described.	-
dc.language.iso	en	en
dc.publisher	Gordon and Breach, Science Publishers Ltd.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1971ApL.....8..115S	en
dc.subject	Time Splitting: Decameter	en
dc.subject	Solar Radio Bursts	en
dc.title	The time splitting of decameter solar radio bursts	en
dc.type	Article	en
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