Estimation of magnetic field components in prominence using magneto hydrodynamic model

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4386

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DC Field	Value	Language
dc.contributor.author	Nagabhushana, B. S	-
dc.date.accessioned	2009-03-05T16:23:59Z	-
dc.date.available	2009-03-05T16:23:59Z	-
dc.date.issued	1999	-
dc.identifier.citation	K.N. Nagendra and J.O. Stenflo., ed., Solar polarization : proceedings of an international workshop held in Bangalore, India, 12 - 16 October, 1998, pp. 421 - 429	en
dc.identifier.isbn	0-7923-5814-7	-
dc.identifier.uri	http://hdl.handle.net/2248/4386	-
dc.description	Restricted Access	-
dc.description.abstract	In this paper we have constructed a quasi two-dimensional model for solar prominence, which is an both magneto-hydrostatic and thermal equilibrium. It is found that the nature of the solution depends on the value of temperature at the center of the prominence (To) and the value of R (the ratio of magnetic pressure at the center of the prominence (pm) to the value of total pressure inside the prominence (C1) The effect of variation of To/sub1 C/sub1 and R on the components of the magnetic field is also discussed.	-
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.ispartofseries	Astrophysics and Space Science Library;Vol. 243	-
dc.relation.uri	http://adsabs.harvard.edu/abs/1999ASSL..243..421N	en
dc.subject	Magnetic field	en
dc.subject	Magneto hydrodynamic model	en
dc.title	Estimation of magnetic field components in prominence using magneto hydrodynamic model	en
dc.type	Article	en
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