萤火虫
发表于 2025-3-28 15:10:22
rption and emission wavelengths. In this arrangement the fluorophores radiate into free space. Most of our knowledge and intuition about fluorescence is derived from the spectral properties observed in these free-space conditions. However, the presence of nearby metallic surfaces or particles can al
鞠躬
发表于 2025-3-28 18:56:36
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内部
发表于 2025-3-29 01:14:11
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ARCHE
发表于 2025-3-29 03:32:20
Merry R. Sherman,Fe B. Tuazon,Yee-Wan Stevens,Joseph A. Carlino,En-Mei Niuadiation, which forms an integral part of the radiative heat transfer solver package in cylindrical coordinates. To keep it consistent and understandable with respect to the methods used, this formulation will be named FVM-SLW henceforth. The discretization of the governing equation is presented alo
带来墨水
发表于 2025-3-29 08:23:24
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Schlemms-Canal
发表于 2025-3-29 14:05:06
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沙草纸
发表于 2025-3-29 15:55:26
Allan Munck,Paul M. Guyrehat these photons reach us though different paths, of different lengths. Then it is not true any longer that a moving sphere will be . or . as contracted in the direction of motion. We will derive that a sphere is seen rotated… and not contracted, since a rotated sphere does not change its shape. An
Airtight
发表于 2025-3-29 23:40:05
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试验
发表于 2025-3-30 02:03:19
George P. Chrousos,D. Lynn Loriaux,Masako Tomita,David D. Brandon,David Renquist,Barry Albertson,Mor 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
COM
发表于 2025-3-30 05:19:43
John W. Funderal 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