Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/4386
Title: | Estimation of magnetic field components in prominence using magneto hydrodynamic model |
Authors: | Nagabhushana, B. S |
Keywords: | Magnetic field Magneto hydrodynamic model |
Issue Date: | 1999 |
Publisher: | Kluwer Academic Publishers |
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 |
Series/Report no.: | Astrophysics and Space Science Library;Vol. 243 |
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. |
Description: | Restricted Access |
URI: | http://hdl.handle.net/2248/4386 |
ISBN: | 0-7923-5814-7 |
Appears in Collections: | IIAP Publications |
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Estimation of magnetic field Restricted Access | Restricted Access | 227.89 kB | Adobe PDF | View/Open Request a copy |
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