On the dependence of solar flare occurrence on sunspot polarity

dc.contributor.author	Verma, V. K.
dc.contributor.author	Shelke, R. N.
dc.date.accessioned	2010-03-03T10:26:08Z
dc.date.available	2010-03-03T10:26:08Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded from ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/601
dc.description.abstract	The possibility of predicting flare occurence on the sun has been examined. It is noticed that the p-polarity dominant spot groups. This high productivity of p-polarity dominant spot groups has been interpreted in terms of (i) high rates of new magnetic flux eruption within the triggering flared (cf. Heyvaerts et al. 1977). Moreever, the productivities of all group types are dependent on the magnetic field strength of the spot froups.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi13-243
dc.subject	Sudden ionospheric disturbances - Solar flares, Sunspot groups, Active region	en_US
dc.title	On the dependence of solar flare occurrence on sunspot polarity	en_US
dc.type	Article	en_US