死亡 发表于 2025-3-30 09:59:32

http://reply.papertrans.cn/17/1637/163684/163684_51.png

addict 发表于 2025-3-30 15:04:20

The Equations of Radiation Hydrodynamicshe equations, and 2) to solve the equations to 0(v/c) in quite general circumstances..These points will be illustrated in the context of the non-equilibrium radiation diffusion limit, and a sketch of how the Lagrangean equations are to be solved will be presented.

信任 发表于 2025-3-30 17:33:04

http://reply.papertrans.cn/17/1637/163684/163684_53.png

天赋 发表于 2025-3-30 23:32:24

Building a Random Quote Generator, symmetry. We also show how to calculate the expected appearance of models for which the source function and extinction coefficient are known. Examples of such calculations are presented and discussed.

冒烟 发表于 2025-3-31 01:01:07

http://reply.papertrans.cn/17/1637/163684/163684_55.png

INCUR 发表于 2025-3-31 07:48:21

https://doi.org/10.1007/978-1-4302-0120-5rtificial viscous “pressure” in the Eulerian equations of motion. These errors are eliminated in the present code, which gives good results on three test problems involving strong relativistic shock waves.

cipher 发表于 2025-3-31 12:00:43

http://reply.papertrans.cn/17/1637/163684/163684_57.png

Expediency 发表于 2025-3-31 16:06:56

Numerical Modeling of Subgrid-Scale Flow in Turbulence, Rotation, and Convectionhich numerical and eddy-viscosities produce incorrect solutions. Improved models of the subgrid-scale flow are examined. We show how numerical simulation of large Reynolds number (but non-turbulent) flows can guide us in modeling subgrid-scale flows in astrophysical settings.
页: 1 2 3 4 5 [6]
查看完整版本: Titlebook: Astrophysical Radiation Hydrodynamics; Karl-Heiz A. Winkler,Michael L. Norman Book 1986 D. Reidel Publishing Company, Dordrecht, Holland 1