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An introduction to radiative transfer : methods and applications in astrophysics /
Astrophysicists have developed several very different methodologies for solving the radiative transfer equation. An Introduction to Radiative Transfer presents these techniques as applied to stellar atmospheres, planetary nebulae, and other objects with similar geometrical and physical conditions.
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Cambridge ; New York :
Cambridge University Press,
2002.
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| Temas: | |
| Acceso en línea: | Texto completo |
MARC
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| 100 | 1 | |a Peraiah, Annamaneni, |d 1937- |1 https://id.oclc.org/worldcat/entity/E39PCjKwcrJJJYBCGmkxhW6PYq | |
| 245 | 1 | 3 | |a An introduction to radiative transfer : |b methods and applications in astrophysics / |c Annamaneni Peraiah. |
| 260 | |a Cambridge ; |a New York : |b Cambridge University Press, |c 2002. | ||
| 300 | |a 1 online resource (xii, 480 pages) : |b illustrations | ||
| 336 | |a text |b txt |2 rdacontent | ||
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| 504 | |a Includes bibliographical references and index. | ||
| 588 | 0 | |a Print version record. | |
| 505 | 0 | 0 | |g Ch. 1. |t Definitions of fundamental quantities of the radiation field -- |g Ch. 2. |t The equation of radiative transfer -- |g Ch. 3. |t Methods of solution of the transfer equation -- |g Ch. 4. |t Two-point boundary problems -- |g Ch. 5. |t Principle of invariance -- |g Ch. 6. |t Discrete space theory -- |g Ch. 7. |t Transfer equation in moving media: the observer frame -- |g Ch. 8. |t Radiative transfer equation in the comoving frame -- |g Ch. 9. |t Escape probability methods -- |g Ch. 10. |t Operator perturbation methods -- |g Ch. 11. |t Polarization -- |g Ch. 12. |t Polarization in magnetic media -- |g Ch. 13. |t Multi-dimensional radiative transfer. |
| 520 | |a Astrophysicists have developed several very different methodologies for solving the radiative transfer equation. An Introduction to Radiative Transfer presents these techniques as applied to stellar atmospheres, planetary nebulae, and other objects with similar geometrical and physical conditions. | ||
| 590 | |a ProQuest Ebook Central |b Ebook Central Academic Complete | ||
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| 650 | 0 | |a Radiative transfer. | |
| 650 | 0 | |a Stars |x Radiation. | |
| 650 | 6 | |a Transfert radiatif. | |
| 650 | 6 | |a Rayonnement stellaire. | |
| 650 | 7 | |a SCIENCE |x Astronomy. |2 bisacsh | |
| 650 | 7 | |a Radiative transfer |2 fast | |
| 650 | 7 | |a Stars |x Radiation |2 fast | |
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| 650 | 7 | |a Strahlungstransport |2 gnd | |
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| 650 | 7 | |a Transfert radiatif. |2 ram | |
| 650 | 7 | |a Rayonnement stellaire. |2 ram | |
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