On the dependence of solar flare occurrence on sunspot polarity

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/659

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DC Field	Value	Language
dc.contributor.author	Verma, V. K	-
dc.contributor.author	Shelke, R. N	-
dc.date.accessioned	2005-12-08T03:51:49Z	-
dc.date.available	2005-12-08T03:51:49Z	-
dc.date.issued	1985-09	-
dc.identifier.citation	BASI, Vol. 13, No. 3, pp. 243-252	en
dc.identifier.uri	http://hdl.handle.net/2248/659	-
dc.description.abstract	The possibility of predicting flare occurrence on the sun has been examined. It is noticed that the p-polarity dominant spot groups are more productive of flares than the f-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 p-polarity dominant spot groups, and (ii) newly erupted magnetic flux triggering flares (cf. Heyvaerts et al. 1977). Moreover, the productivities of all group types are dependent on the magnetic field strength of the spot groups.	en
dc.format.extent	774003 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	Sudden ionospheric disturbances	en
dc.subject	Solar flare	en
dc.subject	Sunspot groups	en
dc.subject	Active region	en
dc.title	On the dependence of solar flare occurrence on sunspot polarity	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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