NEX
发表于 2025-3-27 00:16:31
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Resign
发表于 2025-3-27 04:51:43
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fatuity
发表于 2025-3-27 06:17:02
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Charitable
发表于 2025-3-27 11:47:35
https://doi.org/10.1007/978-3-319-22759-7ave (and will ever have) about distant objects (exceptions are detected neutrinos from the Sun and supernova SN1987a, and in a near future the gravitational waves). However, there is an even more compelling reason for the a need to deal with detailed radiation transport in astrophysics: In many astr
Feedback
发表于 2025-3-27 15:44:38
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有恶意
发表于 2025-3-27 20:08:50
Marco Hübner,Philipp Jahn,Gregor Tewaaggime. We consider the non-relativistic regime to be characterized by material velocities less than or equal to one percent of the speed of light. In most applications, the radiative transfer equations are coupled to the hydrodynamics equations. We first describe a radiation-hydrodynamics model that
Exploit
发表于 2025-3-27 23:11:46
Advances in Production Technologycludes the mean-free-path, one can use an effective propagation kernel that will necessarily be sub-exponential. We come to this conclusion using both standard transport theory for variable media and a point-process approach developed recently by A. Kostinski. The ramifications of this finding for m
敌意
发表于 2025-3-28 02:27:34
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WITH
发表于 2025-3-28 09:43:53
Wolfgang Schulz,Toufik Al Khawlich as Monte Carlo , or SHDOM . However, it is usually required too much time to make a simulation which is inconvenient when just we need an answer on a simple question like how significant the 3D effects are for a given problem. The perturbation method is what comes to mind first if we need
努力赶上
发表于 2025-3-28 14:24:56
https://doi.org/10.1007/978-3-319-12304-2f four possible canopy reflectance models. The overview is followed by the description of the . coupled leaf/canopy turbid medium reflectance model based on natural averaging. The model follows conventional radiative transfer theory with modification for canopy architecture as characterized by leaf