Magnetic Shear and Flares

dc.contributor.author	Venkatakrishnan, P
dc.date.accessioned	2008-09-10T15:23:26Z
dc.date.available	2008-09-10T15:23:26Z
dc.date.issued	1990
dc.identifier.citation	IAU Symposium, No. 142, pp. 319 - 322	en
dc.identifier.issn	0074-1809
dc.identifier.uri	http://hdl.handle.net/2248/3536
dc.description.abstract	Magnetic tension possesses low values at regions of large magnetic “shear” on the polarity inversion line. The low tension allows for a non-force-free field that depends on the density may then possibly evolve into solar flares. Heuristic arguments are given to favour instability driven flare scenarios.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990IAUS..142..319V	en
dc.subject	Magnetic Shear	en
dc.subject	Flares	en
dc.title	Magnetic Shear and Flares	en
dc.type	Article	en