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 |