The Cosmic Ray Flare of March 7, 1942

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/839

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.contributor.author	Punetha, L. M	-
dc.date.accessioned	2006-04-06T09:48:21Z	-
dc.date.available	2006-04-06T09:48:21Z	-
dc.date.issued	1966-11	-
dc.identifier.citation	KOB No 179	en
dc.identifier.uri	http://hdl.handle.net/2248/839	-
dc.description.abstract	The variation of the dynamic characteristics of the cosmic ray limb flare of March 7, 1942 based on the K/sub232/ spectroheliograms and H-alpha spectrohelioscope observations of Kodaikanal is presented. Although the flare had high flare ribbon velocities of the order of 17 km/sec. during the flash phase, with subsequent changes in its configuration, its effect on the nearby prominence was trival. The loop prominence with typical condensations and knots formed at a height of 30,000 km. above the limb and connected to the chromosphere by thin curved threads was noticed, about 1 1/2 hours after the flash phase	en
dc.format.extent	213578 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Kodaikanal Observatory	en
dc.subject	Cosmic Ray Flare	en
dc.title	The Cosmic Ray Flare of March 7, 1942	en
dc.type	Article	en
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