Book Description
An essential overview of the physical and mathematical background of radiative transfer, and its applications to stellar and planetary atmospheres.
Author : Lucio Crivellari
Publisher : Cambridge University Press
Page : 251 pages
File Size : 27,59 MB
Release : 2020-01-09
Category : Science
ISBN : 1108499538
An essential overview of the physical and mathematical background of radiative transfer, and its applications to stellar and planetary atmospheres.
Author : Subrahmanyan Chandrasekhar
Publisher : Courier Corporation
Page : 418 pages
File Size : 41,88 MB
Release : 2013-04-15
Category : Science
ISBN : 0486318451
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.
Author : Ivan Hubeny
Publisher : Princeton University Press
Page : 944 pages
File Size : 44,66 MB
Release : 2014-10-26
Category : Science
ISBN : 0691163294
The most authoritative synthesis of the quantitative spectroscopic analysis of stellar atmospheres This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the observable outer layers of stars and similar objects. Written by two leading researchers in the field, it presents a comprehensive account of both the physical foundations and numerical methods of such analyses. The book is ideal for astronomers who want to acquire deeper insight into the physical foundations of the theory of stellar atmospheres, or who want to learn about modern computational techniques for treating radiative transfer in non-equilibrium situations. It can also serve as a rigorous yet accessible introduction to the discipline for graduate students. Provides a comprehensive, up-to-date account of the field Covers computational methods as well as the underlying physics Serves as an ideal reference book for researchers and a rigorous yet accessible textbook for graduate students An online illustration package is available to professors at press.princeton.edu
Author : Lucio Crivellari
Publisher :
Page : pages
File Size : 17,59 MB
Release : 2020
Category : Planets
ISBN : 9781108730792
"Radiative transfer is essential for obtaining information from the spectra of astrophysical objects. This volume provides an overview of the physical and mathematical background of radiative transfer, and its applications to stellar and planetary atmospheres. It covers the phenomenology and physics of early-type and late-type stars, as well as ultra-cool dwarf stars and extrasolar planets"--
Author : Annamaneni Peraiah
Publisher : Cambridge University Press
Page : 494 pages
File Size : 23,56 MB
Release : 2002
Category : Science
ISBN : 9780521770019
This 2001 book presents the methodologies used by astrophysicists for solving the radiative transfer equation.
Author : Henny J. G. L. M. Lamers
Publisher : Cambridge University Press
Page : 456 pages
File Size : 10,39 MB
Release : 1999-06-17
Category : Nature
ISBN : 9780521595650
The first comprehensive introduction to the observations and theories of stellar winds; a long-awaited graduate textbook, written by two founders of the field.
Author : George B. Rybicki
Publisher : John Wiley & Sons
Page : 402 pages
File Size : 13,49 MB
Release : 2008-09-26
Category : Science
ISBN : 352761818X
Radiative Processes in Astrophysics: This clear, straightforward, and fundamental introduction is designed to present-from a physicist's point of view-radiation processes and their applications to astrophysical phenomena and space science. It covers such topics as radiative transfer theory, relativistic covariance and kinematics, bremsstrahlung radiation, synchrotron radiation, Compton scattering, some plasma effects, and radiative transitions in atoms. Discussion begins with first principles, physically motivating and deriving all results rather than merely presenting finished formulae. However, a reasonably good physics background (introductory quantum mechanics, intermediate electromagnetic theory, special relativity, and some statistical mechanics) is required. Much of this prerequisite material is provided by brief reviews, making the book a self-contained reference for workers in the field as well as the ideal text for senior or first-year graduate students of astronomy, astrophysics, and related physics courses. Radiative Processes in Astrophysics also contains about 75 problems, with solutions, illustrating applications of the material and methods for calculating results. This important and integral section emphasizes physical intuition by presenting important results that are used throughout the main text; it is here that most of the practical astrophysical applications become apparent.
Author : Sara Seager
Publisher : Princeton University Press
Page : 258 pages
File Size : 37,19 MB
Release : 2010-08-02
Category : Science
ISBN : 1400835305
Over the past twenty years, astronomers have identified hundreds of extrasolar planets--planets orbiting stars other than the sun. Recent research in this burgeoning field has made it possible to observe and measure the atmospheres of these exoplanets. This is the first textbook to describe the basic physical processes--including radiative transfer, molecular absorption, and chemical processes--common to all planetary atmospheres, as well as the transit, eclipse, and thermal phase variation observations that are unique to exoplanets. In each chapter, Sara Seager offers a conceptual introduction, examples that combine the relevant physics equations with real data, and exercises. Topics range from foundational knowledge, such as the origin of atmospheric composition and planetary spectra, to more advanced concepts, such as solutions to the radiative transfer equation, polarization, and molecular and condensate opacities. Since planets vary widely in their atmospheric properties, Seager emphasizes the major physical processes that govern all planetary atmospheres. Moving from first principles to cutting-edge research, Exoplanet Atmospheres is an ideal resource for students and researchers in astronomy and earth sciences, one that will help prepare them for the next generation of planetary science. The first textbook to describe exoplanet atmospheres Illustrates concepts using examples grounded in real data Provides a step-by-step guide to understanding the structure and emergent spectrum of a planetary atmosphere Includes exercises for students
Author : C. J. Schrijver
Publisher : Cambridge University Press
Page : 404 pages
File Size : 21,42 MB
Release : 2008-10-30
Category : Science
ISBN : 1139425420
This timely volume provides the first comprehensive review and synthesis of current understanding of magnetic fields in the Sun and similar stars. Magnetic activity results in a wealth of phenomena - including starspots, non-radiatively heated outer atmospheres, activity cycles, deceleration of rotation rates, and even, in close binaries, stellar cannibalism - all of which are covered clearly and authoritatively. This book brings together for the first time recent results in solar studies and stellar studies. The result is an illuminating new view of stellar magnetic activity. Key topics include radiative transfer, convective simulations, dynamo theory, outer-atmospheric heating, stellar winds and angular momentum loss. Researchers are provided with a state-of-the-art review of this exciting field, and the pedagogical style and introductory material make the book an ideal and welcome introduction for graduate students.
Author : Gary E. Thomas
Publisher : Cambridge University Press
Page : 554 pages
File Size : 34,95 MB
Release : 2002-01-28
Category : Nature
ISBN : 9780521890618
Provides a foundation of the theoretical and practical aspects of radiative transfer, for the atmospheric, oceanic and environmental sciences.