Some features of geomagnetic sudden commencements following cosmic ray flares

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5128

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DC Field	Value	Language
dc.contributor.author	Bhargava, B. N	-
dc.contributor.author	Subrahmanyan, R. V	-
dc.date.accessioned	2010-06-02T09:54:29Z	-
dc.date.available	2010-06-02T09:54:29Z	-
dc.date.issued	1966-09	-
dc.identifier.citation	Planetary and Space Science, Vol. 14, pp. 871 - 889	en
dc.identifier.issn	0032-0633	-
dc.identifier.uri	http://hdl.handle.net/2248/5128	-
dc.description	Restricted Access	-
dc.description.abstract	The amplitudes of geomagnetic sudden commencements are examined in ion to the optical, energetic particle and radio characteristics of source flares. It has been shown that all sudden commencements of amplitude above a threshold minimum at a given middle latitude station are associated with energetic particle events. East-west asymmetry and centre-limb variation in propagation times of storm plasma have also been examined. The day-time enhancement of SC amplitudes in the equatorial regions has been briefly discussed. The SC amplitude characteristics have been utilized to identify about 50 solar proton events during sunspot cycles 12–18.	en
dc.language.iso	en	en
dc.publisher	Pergamon Press	en
dc.relation.uri	http://dx.doi.org/10.1016/0032-0633(66)90093-6	en
dc.rights	© Pergamon Press	en
dc.title	Some features of geomagnetic sudden commencements following cosmic ray flares	en
dc.type	Article	en
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