| 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 |