Numerical solution of the radiation transport equation in disk geometry
- 30 June 1987
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 37 (6) , 565-580
- https://doi.org/10.1016/0022-4073(87)90060-4
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- DUSTCD: A radiative transport code for spherically symmetric dust cloudsComputer Physics Communications, 1983
- The Physical Effects of Radiative Transfer in Multidimensional Media Including Models of the Solar AtmosphereThe Astrophysical Journal Supplement Series, 1980
- Two-dimensional radiative transfer. I - Planar geometryThe Astrophysical Journal, 1978
- Numerical solution of the radiative transfer equation in spherically symmetric dust shellsJournal of Quantitative Spectroscopy and Radiative Transfer, 1976
- Radiation transport in dense interstellar dust clouds. I - Grain temperatureThe Astrophysical Journal, 1975
- Theory of extended stellar atmospheres. I - Computational method and first results for static spherical modelsThe Astrophysical Journal Supplement Series, 1974
- Numerical evaluation of the formal solution of radiative transfer problems in spherical geometriesComputer Physics Communications, 1973
- The stellar atmospheres problemJournal of Quantitative Spectroscopy and Radiative Transfer, 1971
- Radiative Transfer in Spherically Symmetric Systems. The Conservative Grey CaseMonthly Notices of the Royal Astronomical Society, 1971
- On the Use of Variable Eddington Factors in Non-LTE Stellar Atmospheres ComputationsMonthly Notices of the Royal Astronomical Society, 1970