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Cambridge University Press - An Introduction to Radiative Transfer

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Description

Master the complex methodologies used by astrophysicists to solve the radiative transfer equation. This comprehensive text from Cambridge University Press provides a deep look into various techniques applied to stellar atmospheres, planetary nebulae, supernovae, and other celestial objects with similar physical conditions. Readers will explore a wide range of approaches, including accurate, fast, probabilistic, and approximate methods. The book covers the latest and most advanced techniques available in the field today. Whether you are studying line profiles or the complexities of polarization, this resource provides the necessary mathematical and physical frameworks. It specifically addresses polarization due to resonance line scattering and polarization in various astrophysical contexts, making it an essential reference for researchers and students in astronomy and space science.

Key Features

https://www.amazon.co.uk/dp/B0GFY1Z5MG?tag=tosheroon-21

Applies theoretical techniques to real-world objects like stellar atmospheres, supernovae, and planetary nebulae.

Includes a variety of computational approaches such as accurate, fast, probabilistic, and approximate methods.

Provides access to the latest and most advanced techniques currently used in the scientific community.

Explains specialized topics including line profile computation and polarization due to resonance line scattering.

Detailed analysis of polarization in different astrophysical environments and physical conditions.

Product Specifications

Format
paperback
Domain
Amazon UK
Release Date
05 January 2010
Listed Since
22 January 2007

Barcode

No barcode data available

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