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Titlebook: Radiative Transfer; An Introduction to E Hélène Frisch Book 2022 The Editor(s) (if applicable) and The Author(s), under exclusive license t

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發(fā)表于 2025-3-21 19:11:09 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Radiative Transfer
副標(biāo)題An Introduction to E
編輯Hélène Frisch
視頻videohttp://file.papertrans.cn/821/820525/820525.mp4
概述A single volume for several exact methods of solution applicable in Astrophysics and Physics.Solutions of scalar, vector, and matrix Cauchy singular integral equations.The density matrix and the class
圖書(shū)封面Titlebook: Radiative Transfer; An Introduction to E Hélène Frisch Book 2022 The Editor(s) (if applicable) and The Author(s), under exclusive license t
描述.This book discusses analytic and asymptotic methods relevant to radiative transfer in dilute media, such as stellar and planetary atmospheres.??Several methods, providing exact expressions for the radiation field in a semi-infinite atmosphere, are described in detail and applied to unpolarized and polarized continuous spectra and spectral lines. Among these methods, the Wiener–Hopf method, introduced in 1931 for a stellar atmospheric problem, is used today in fields such as solid mechanics, diffraction theory, or mathematical finance. Asymptotic analyses are carried out on unpolarized and polarized radiative transfer equations and on a discrete time random walk. Applicable when photons undergo a large number of scatterings, they provide criteria to distinguish between large-scale diffusive and non-diffusive behaviors, typical scales of variation of the radiation field, such as the thermalization length, and specific descriptions for regions close and far from boundaries.?..Its well organized synthetic view of exact and asymptotic methods of radiative transfer makes this book a valuable resource for both graduate students and professional scientists in astrophysics and beyond..
出版日期Book 2022
關(guān)鍵詞analytical solution of radiative transfer; exact calculation of radiative transfer; Radiative transfer
版次1
doihttps://doi.org/10.1007/978-3-030-95247-1
isbn_softcover978-3-030-95249-5
isbn_ebook978-3-030-95247-1
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl
The information of publication is updating

書(shū)目名稱Radiative Transfer影響因子(影響力)




書(shū)目名稱Radiative Transfer影響因子(影響力)學(xué)科排名




書(shū)目名稱Radiative Transfer網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Radiative Transfer網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




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沙發(fā)
發(fā)表于 2025-3-21 21:32:32 | 只看該作者
Conservative Scattering: The Milne Problemion obtained in Chap. . to derive an exact expression of the source function. For monochromatic scattering, we show how to express it in terms of the Hopf function and describe the properties of the latter.
板凳
發(fā)表于 2025-3-22 03:07:16 | 只看該作者
The Case Eigenfunction Expansion Method The eigenfunctions are used to expand arbitrary solutions, and the main task consists of the determination of the expansion coefficients. In this Chapter, this method referred as the Case expansion method, is applied to radiative transfer equations for monochromatic scattering and complete frequency redistribution.
地板
發(fā)表于 2025-3-22 07:35:27 | 只看該作者
The ,-law and the Nonlinear ,-Equationey do not make use of complex plane analysis, whether they are really elementary, is a matter of appreciation. A certain advantage of these methods is that there is in general no need to distinguish between monochromatic scattering and complete frequency redistribution.
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Conservative Rayleigh Scattering: Exact Solutionsne (a matrix Riemann–Hilbert problem), which is then decomposed into two scalar Riemann–Hilbert problems. The decomposition method closely follows the 1967 approach of C. Siewert and S. Fraley. The two scalar problems, solved with the method described in Chapter 5, provide the functions ..(.) and ..(.).
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Book 2022al methods, providing exact expressions for the radiation field in a semi-infinite atmosphere, are described in detail and applied to unpolarized and polarized continuous spectra and spectral lines. Among these methods, the Wiener–Hopf method, introduced in 1931 for a stellar atmospheric problem, is
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發(fā)表于 2025-3-23 05:45:50 | 只看該作者
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