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Radiative Transfer is the definitive work in the field. It provides workers and students in physics, nuclear physics, astrophysics, and atmospheric studies with the foundation for the analysis of stellar atmospheres, planetary illumination, and sky radiation. Though radiative transfer has been investigated chiefly as a phenomenon of astrophysics, in recent years it has attracted the attentions of physicists as well, since essentially the same problems arise in the theory of diffusion of neutrons.' Morton D. Hall, Distinguished Service Professor, University of ChicagoChandrasekhar presents the subject of radiative transfer in planeparallel atmosphere as a branch of mathematical physics, with its own characteristic methods and techniques. He begins with a formulation and analysis of fundamental problems. It is shown how allowance can be made for the polarization of the radiation field by using a set of parameters first introduced by Stokes. Successive chapters deal with transfer problems in semiinfinite and finite atmosphere; Rayleigh scattering; the radiative equilibrium of a stellar atmosphere; and related astrophysical and mathematical problems. The mathematical methods employed are extremely powerful, and by means of them it has been possible to handle problems which could not be treated previously, such as the scattering of polarized light.
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- Q: What is the primary focus of the book 'Radiative Transfer'? A: 'Radiative Transfer' focuses on the analysis of radiative transfer phenomena in various fields such as physics, astrophysics, and atmospheric studies.
- Q: Who is the author of 'Radiative Transfer'? A: The book is authored by S. Chandrasekhar, a renowned physicist known for his significant contributions to the field.
- Q: What topics are covered in 'Radiative Transfer'? A: The book covers topics such as stellar atmospheres, planetary illumination, sky radiation, Rayleigh scattering, and the radiative equilibrium of stellar atmospheres.
- Q: Is 'Radiative Transfer' suitable for students? A: Yes, 'Radiative Transfer' is suitable for both students and professionals in the fields of physics and astrophysics, providing foundational knowledge in radiative transfer.
- Q: What is the publication date of 'Radiative Transfer'? A: 'Radiative Transfer' was originally published on January 1, 1960, and was re-released on June 21, 2011.
- Q: How many pages does 'Radiative Transfer' have? A: 'Radiative Transfer' contains a total of 416 pages.
- Q: What type of binding does 'Radiative Transfer' have? A: 'Radiative Transfer' is available in paperback binding.
- Q: What is the condition of the book 'Radiative Transfer'? A: 'Radiative Transfer' is classified as 'New', ensuring that it has not been previously used or damaged.
- Q: Does 'Radiative Transfer' include advanced mathematical methods? A: Yes, the book employs advanced mathematical methods to address complex problems in radiative transfer.
- Q: What makes 'Radiative Transfer' a definitive work in its field? A: 'Radiative Transfer' is considered definitive due to its comprehensive analysis and the introduction of key concepts related to radiative transfer phenomena.