Book contents
- Frontmatter
- Contents
- List of Contributors
- Preface
- Acknowledgements
- 1 The Physical Grounds of Radiative Transfer
- 2 Fundamental Physical Aspects of Radiative Transfer
- 3 Numerical Methods in Radiative Transfer
- 4 Stellar Atmosphere Codes
- 5 Radiative Transfer in the (Expanding) Atmospheres of Early-Type Stars, and Related Problems
- 6 Phenomenology and Physics of Late-Type Stars
- 7 Modelling the Atmospheres of Ultracool Dwarfs and Extrasolar Planets
4 - Stellar Atmosphere Codes
Published online by Cambridge University Press: 24 December 2019
- Frontmatter
- Contents
- List of Contributors
- Preface
- Acknowledgements
- 1 The Physical Grounds of Radiative Transfer
- 2 Fundamental Physical Aspects of Radiative Transfer
- 3 Numerical Methods in Radiative Transfer
- 4 Stellar Atmosphere Codes
- 5 Radiative Transfer in the (Expanding) Atmospheres of Early-Type Stars, and Related Problems
- 6 Phenomenology and Physics of Late-Type Stars
- 7 Modelling the Atmospheres of Ultracool Dwarfs and Extrasolar Planets
Summary
A description is given of stellar atmosphere codes – both codes for calculating the structure of the stellar atmosphere (i.e., including an energy equation) and codes for calculating the emergent spectrum from a given atmospheric structure. Emphasis has been given to codes that are either publicly available or in wide use by a large community. References are given for detailed code descriptions and for typical applications of the codes.
- Type
- Chapter
- Information
- Radiative Transfer in Stellar and Planetary Atmospheres , pp. 117 - 150Publisher: Cambridge University PressPrint publication year: 2020