Published 1972
| Version v1
Journal article
The Eddington factor for radiative transfer in spherical geometry
Description
The present paper shows that, contrary to the statement of Hummer & Rybicki, the half-range method (Wilson & Sen) can handle the outward peaking effect of the radiation field in extensive spherical media. The source function J ( r ) and the Eddington factor f ( r ) = [ K ( r )/ J ( r )] have been calculated by the half-range method with k ( r ) = r−2 for o < r ≼ R , where R = 3 and R = 10. The values for R = 10 are compared with those of Hummer & Rybicki and are found to be in fairly good agreement.
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 160
- Journal Issue
- 4
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 349-353
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 4057894
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BOUNDARY CONDITIONS; DISTRIBUTION; ENERGY TRANSFER; FUNCTIONS; GEOMETRY; ITERATIVE METHODS; LAYERS; NUMERICAL SOLUTION; PEAKS; RADIATIONS; SPHERES; SPHERICAL CONFIGURATION; SPHERICAL HARMONICS METHOD; STARS; STELLAR ATMOSPHERES
- Descriptors DEC
- ATMOSPHERES; CONFIGURATION; MATHEMATICS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent