dc.contributor.author |
Peraiah, A |
|
dc.date.accessioned |
2005-05-18T09:55:29Z |
|
dc.date.available |
2005-05-18T09:55:29Z |
|
dc.date.issued |
1986-05 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 5, No. 2, pp. 113-140 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/403 |
|
dc.description.abstract |
We present details of a new technique of obtaining a numerical solution of the radiative transfer equation in spherical symmetry in a polychromatic system. We employed the integral operators together with an interpolation formula of the specific intensity defined on radius-angle-frequency grid. We found that the method is quite stable and employs a large stepsize in all the variables on the grid. We employed complete redistribution in calculating the lines |
en |
dc.format.extent |
1047293 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
Spectral lines |
en |
dc.subject |
Radiative transfer equation in spherical symmetry |
en |
dc.title |
Integral Operator Technique of Line Transfer |
en |
dc.type |
Article |
en |