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標(biāo)題: Titlebook: Radiative Transfer; An Introduction to E Hélène Frisch Book 2022 The Editor(s) (if applicable) and The Author(s), under exclusive license t [打印本頁]

作者: Fillmore    時間: 2025-3-21 19:11
書目名稱Radiative Transfer影響因子(影響力)




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




書目名稱Radiative Transfer網(wǎng)絡(luò)公開度




書目名稱Radiative Transfer網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Radiative Transfer被引頻次




書目名稱Radiative Transfer被引頻次學(xué)科排名




書目名稱Radiative Transfer年度引用




書目名稱Radiative Transfer年度引用學(xué)科排名




書目名稱Radiative Transfer讀者反饋




書目名稱Radiative Transfer讀者反饋學(xué)科排名





作者: Dissonance    時間: 2025-3-21 21:32
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.
作者: restrain    時間: 2025-3-22 03:07
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.
作者: 確定的事    時間: 2025-3-22 07:35
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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作者: 無目標(biāo)    時間: 2025-3-23 05:03
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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作者: 食物    時間: 2025-3-23 13:13
An Overview of the Content,Part II to their generalization to vector and matrix problems for linearly polarized radiation fields. In Part I we deal only with the radiation field intensity, whereas in Part II we also consider the linear polarization created by the scattering of photons. In Part III, we use asymptotic methods t
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作者: Antioxidant    時間: 2025-3-23 21:54
Exact Methods of Solution: A Brief Surveys chapter we present, more or less in a chronological order, a brief summary of exact methods of solution. They are described in detail in the next chapters, following an inverse chronological order, recent methods allowing us to introduce tools and concepts that make it easier to understand the fir
作者: 小步舞    時間: 2025-3-23 22:22
Singular Integral Equations exact methods of solutions have been developed, in other branches of physics or in mathematical physics. For infinite media, as shown in Sect. ., the integral equation for the source function can be transformed into an algebraic equation by performing a Fourier transform. For radiative transfer pro
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作者: 懦夫    時間: 2025-3-24 16:00
Spectral Line with Continuous Absorptions such as the Sun the dominant source of continuous absorption is the negative hydrogen ion H., an ion with a single bound state of low binding energy. In this Chapter we show how a continuous absorption and a continuous emission modify the results presented in Chap. . for spectral lines formed with
作者: 犬儒主義者    時間: 2025-3-24 20:10

作者: Apoptosis    時間: 2025-3-25 00:14
The Case Eigenfunction Expansion Methodier approach to partial differential equations. The basic idea is to construct a set of eigenfunctions, solutions of a homogeneous transport equation. The eigenfunctions are used to expand arbitrary solutions, and the main task consists of the determination of the expansion coefficients. In this Cha
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作者: EVEN    時間: 2025-3-25 18:03
Polarized Radiative Transfer Equationsolev. In this chapter, we present a few linearly polarized radiative transfer equations describing monochromatic Rayleigh scattering, resonance polarization, and the Hanle effect, and then show how to construct vector and matrix convolution integral equations. They are used, in the following chapter
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作者: 十字架    時間: 2025-3-26 05:15
Scattering Problems with No Exact Solution I: The Auxiliary Matricesresonance polarization, and the Hanle effect. For these processes, there is no explicit solution for radiative transfer problems in semi-infinite plane parallel media. They have to be solved numerically, directly from the radiative transfer equations, or by means of a nonlinear .-equation. The funda
作者: anachronistic    時間: 2025-3-26 09:45

作者: construct    時間: 2025-3-26 13:20
Radiative Transfer Equations presented in Appendix J of Chap. . and some asymptotic results on the large scale behavior of the radiation field in Chap. .. Otherwise, we consider only spectral lines formed with complete frequency redistribution (also known as .) for which exact results can be obtained.
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作者: 認識    時間: 2025-3-28 15:59
Hélène Frischtical suggestions of ways to support young children’s inquiry learning. Drawing on pedagogy and research from around the world, this book will be of interest toscholars of STEAM education, early childhood educators, students of early childhood education and parents of young children..978-3-030-65626-3978-3-030-65624-9
作者: 凝乳    時間: 2025-3-28 20:27
ts 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..978-3-030-95249-5978-3-030-95247-1
作者: ascetic    時間: 2025-3-28 23:27

作者: Palpate    時間: 2025-3-29 04:45
Book 2022alization 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..
作者: Trochlea    時間: 2025-3-29 07:55
romises to revolutionize life much more profoundly than elevators, electric motors or even personal computer evolution ever did. The EUC 2004 conference provided a forum for engineers and scientists in academia, industry, and government to address all the resulting profound ch- lenges including tech
作者: 學(xué)術(shù)討論會    時間: 2025-3-29 11:48

作者: coltish    時間: 2025-3-29 16:22
Hélène Frischm resources. To avoid that the critical business processes in ERP systems are negatively affected from excessive hardware consumption, we suggest scaling out this category of use cases to corresponding AI technology platform and called side-by-side artificial intelligence. While we focus in this cha
作者: DAUNT    時間: 2025-3-29 23:00
Hélène Frischm resources. To avoid that the critical business processes in ERP systems are negatively affected from excessive hardware consumption, we suggest scaling out this category of use cases to corresponding AI technology platform and called side-by-side artificial intelligence. While we focus in this cha
作者: Dissonance    時間: 2025-3-30 01:45
Hélène Frischm resources. To avoid that the critical business processes in ERP systems are negatively affected from excessive hardware consumption, we suggest scaling out this category of use cases to corresponding AI technology platform and called side-by-side artificial intelligence. While we focus in this cha
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作者: 符合規(guī)定    時間: 2025-3-31 03:16
Hélène Frischutives can use in this quest, which is aimed at providing society with economic and ecological benefits and, whenever possible, the simultaneous provision of these benefits in the form of mutualistic economizing or triple bottom-line business. According to Chapter 6, the ability of executives to act




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