RADIATIVE TRANSFER IN EXTENDED STELLAR ATMOSPHERES,
Abstract
To investigate the transfer of radiation in extended stellar atmospheres, the transfer equation is solved for an infinite spherically symmetric medium by expanding the intensity in terms of Legendre polynomials. The nature of the solutions is discussed in detail. A literature survey and a presentation of the basic theory are included. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Jun 01, 1964
- Accession Number
- AD0456085
Entities
People
- Robert Dewitt Chapman
Organizations
- Harvard College