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Radiative Transfer S. Chandrasekhar

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Book Title
Radiative Transfer
ISBN
9780486605906

關於產品

Product Identifiers

Publisher
Dover Publications, Incorporated
ISBN-10
0486605906
ISBN-13
9780486605906
eBay Product ID (ePID)
1039089

Product Key Features

Number of Pages
416 Pages
Publication Name
Radiative Transfer
Language
English
Subject
Physics / Astrophysics, Mechanics / Thermodynamics
Publication Year
2011
Type
Textbook
Author
S. Chandrasekhar
Subject Area
Science
Series
Dover Books on Physics Ser.
Format
Trade Paperback

Dimensions

Item Height
0.8 in
Item Weight
17.4 Oz
Item Length
8.5 in
Item Width
5.4 in

Additional Product Features

Intended Audience
College Audience
Illustrated
Yes
Dewey Decimal
523.01
Synopsis
This book by a Nobel Laureate provides the foundation for analysis of stellar atmospheres, planetary illumination, and sky radiation. Suitable for students and professionals in physics, nuclear physics, astrophysics, and atmospheric studies. 1950 edition., " 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 Chicago Chandrasekhar presents the subject of radiative transfer in plane-parallel 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 semi-infinite 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., This book by a Nobel Laureate provides the foundation for analysis of stellar atmospheres, planetary illumination, and sky radiation. Radiation transfer has been investigated as a phenomenon of astrophysics, and it has attained wider interest because of similar problems in the theory of neutron diffusion. Suitable for students and professionals in physics, nuclear physics, astrophysics, and atmospheric studies. 1950 edition.

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