Fillmore 发表于 2025-3-21 19:11:09
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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.restrain 发表于 2025-3-22 03:07:16
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.确定的事 发表于 2025-3-22 07:35:27
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.钢盔 发表于 2025-3-22 11:14:44
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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 ..(.).cinder 发表于 2025-3-23 00:05:59
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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, ishereditary 发表于 2025-3-23 05:45:50
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