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Transfert radiatif - Livre de poche, par S. Chandrasekhar - Bon état
6,71 USD
Environ5,80 EUR
État :
Bon état
Livre ayant déjà été lu, mais qui est toujours en bon état. La couverture présente des dommages mineurs, comme des éraflures, mais n'est ni trouée ni déchirée. Pour les couvertures rigides, la jaquette n'est pas nécessairement incluse. La reliure présente des marques d'usure mineures. La majorité des pages sont intactes. Pliures et déchirures mineures. Soulignement de texte mineur au crayon. Aucun surlignement de texte. Aucune note dans les marges. Aucune page manquante. Consulter l'annonce du vendeur pour avoir plus de détails et voir la description des défauts.
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Livraison :
Gratuit USPS Media MailTM.
Lieu où se trouve l'objet : Philadelphia, Pennsylvania, États-Unis
Délai de livraison :
Estimé entre le sam. 9 août et le jeu. 14 août à 94104
Retours :
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Numéro de l'objet eBay :146262543835
Dernière mise à jour le 06 août 2025 10:30:06 CEST. Afficher toutes les modificationsAfficher toutes les modifications
Caractéristiques de l'objet
- État
- Book Title
- Radiative Transfer
- ISBN
- 9780486605906
À propos de ce produit
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
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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