Titlebook: Astrophysical Radiation Hydrodynamics; Karl-Heiz A. Winkler,Michael L. Norman Book 1986 D. Reidel Publishing Company, Dordrecht, Holland 1

graphic

書目名稱Astrophysical Radiation Hydrodynamics影響因子(影響力)




書目名稱Astrophysical Radiation Hydrodynamics影響因子(影響力)學(xué)科排名




書目名稱Astrophysical Radiation Hydrodynamics網(wǎng)絡(luò)公開度




書目名稱Astrophysical Radiation Hydrodynamics網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Astrophysical Radiation Hydrodynamics被引頻次




書目名稱Astrophysical Radiation Hydrodynamics被引頻次學(xué)科排名




書目名稱Astrophysical Radiation Hydrodynamics年度引用




書目名稱Astrophysical Radiation Hydrodynamics年度引用學(xué)科排名




書目名稱Astrophysical Radiation Hydrodynamics讀者反饋




書目名稱Astrophysical Radiation Hydrodynamics讀者反饋學(xué)科排名

BATE

難理解

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

復(fù)習(xí)

Astigmatism

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

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

共棲

embolus

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

展覽

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