Excitation of high-m tearing modes at the solar flare site

dc.contributor.author	Krishan, V
dc.date.accessioned	2008-12-16T09:58:48Z
dc.date.available	2008-12-16T09:58:48Z
dc.date.issued	1982-10
dc.identifier.citation	Solar Physics, Vol. 80, No.2, pp. 313 - 316	en
dc.identifier.issn	0038-0938 (Print) 1573-093X (Online)
dc.identifier.uri	http://hdl.handle.net/2248/4066
dc.description	Open Access
dc.description.abstract	It is shown that high-m drift tearing modes can be excited under the conditions prevalent at the solar flare sites. Since the growth rate of the high-m tearing modes is larger than that for low-m macroscopic tearing modes and smaller than that of microscopic ion-acoustic instability, these modes warrant accommodation in the scheme of instabilities possibly operating in the hybrid model of solar flares suggested by Spicer	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Company	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1982SoPh...80..313K	en
dc.relation.uri	http://www.springerlink.com/content/kn367772q447077v/	en
dc.rights	D. Reidel Publishing Company
dc.subject	Solar Flares	en
dc.subject	Tearing Modes (Plasmas)	en
dc.subject	Electron Energy	en
dc.subject	Solar Magnetic Field	en
dc.title	Excitation of high-m tearing modes at the solar flare site	en
dc.type	Article	en