graphic
发表于 2025-3-21 16:38:31
书目名称Astrophysical Radiation Hydrodynamics影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0163684<br><br> <br><br>书目名称Astrophysical Radiation Hydrodynamics读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0163684<br><br> <br><br>
BATE
发表于 2025-3-21 20:52:06
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难理解
发表于 2025-3-22 01:11:53
WH80s: Numerical Radiation Hydrodynamicsve transfer and its moments are formulated in a fully adaptive coordinate system in space, angle and frequency. Integral conservation laws for the radiation quantities, which form the basis for our method, are then given. A hierarchy of splitting schemes for reducing this 3-dimensional problem to on
复习
发表于 2025-3-22 04:53:37
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Astigmatism
发表于 2025-3-22 11:19:09
Implicit 2D-Radiation Hydrodynamics) and by Bodenheimer and Sweigart (1968), due to the conspicuous non-homology of the gravitational collapse of a (non-rotating, non-magnetic) interstellar cloud on the verge of being Jeans-unstable, both time and length scales vary by several orders of magnitude during the evolution of the cloud. To
exclamation
发表于 2025-3-22 15:45:50
2-D Eulerian Hydrodynamics with Fluid Interfaces, Self-Gravity and Rotationamical problems in astrophysics involving inviscid compressible flow, self-gravitation, rotation, and fluid instabilities of the Rayleigh-Taylor and Kelvin-Helmholtz types. The computer code to be described has been applied most recently to modeling jets in radio galaxies (Norman et al. 1981, 1982)
Ganglion-Cyst
发表于 2025-3-22 19:56:39
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共栖
发表于 2025-3-22 22:45:45
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embolus
发表于 2025-3-23 04:55:43
Finite Element Methods for Time Dependent Problemsf methods for solving partial differential equations. Their range of application has expanded inexorably so that they now pervade almost all areas. In certain applications, such as time dependent and fluids problems, finite elements have been in use for only a relatively short period of time and one
展览
发表于 2025-3-23 08:15:52
Description and Philosophy of Spectral Methodsferences. For example, the ∇. operator in 2 or 3 dimensions is easier to invert with spectral techniques because the spatial dependence of the operator separates in a more natural way. We warn against the use of some of the more common spectral expansions. Bessel series expansions of functions in cy