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	2006-04-10T06:43:40Z
dc.date.available	2006-04-10T06:43:40Z
dc.date.issued	1986-06
dc.identifier.citation	BASI, Vol. 14, No. 2, pp. 91-94	en
dc.identifier.uri	http://hdl.handle.net/2248/910
dc.description.abstract	A 'twisting index' is defined, assuming that flares tend to occur in highly sheared magnetic fields which also lead to a twisting of magnetic neutral lines in complex active regions. 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 is noted	en
dc.format.extent	248623 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of Indian	en
dc.subject	Neutral line	en
dc.subject	Twisting index	en
dc.subject	H-alpha flare	en
dc.title	Association of solar flares with twisting of magnetic neutral lines	en
dc.type	Article	en