Association of solar flares with twisting of magnetic neutral lines

dc.contributor.author	Uddin, W.
dc.contributor.author	Pande, M. C.
dc.contributor.author	Shelke, R. N.
dc.date.accessioned	2010-02-16T09:47:41Z
dc.date.available	2010-02-16T09:47:41Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/526
dc.description.abstract	Assuming that the flares tend to occur in highly sheared magnetic fields which also lead to a twisting of magnetic neutral line in complex active regions, we have defined a ‘twisting index’. The correlation of this twisting index with flares of various importance classes has been investigated. For cases where at least one bright flare has occurred in the complex active region the number of flare events seems to increase with the twisting index. For the cases of at least one normal flare or all faint flares, a similar but weaker dependence has been noticed.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	basi14-91
dc.subject	Neutral Line, Twisting Index, H-Alpha Flare	en_US
dc.title	Association of solar flares with twisting of magnetic neutral lines	en_US
dc.type	Article	en_US