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

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期刊全称Astrophysical Radiation Hydrodynamics
影响因子2023Karl-Heiz A. Winkler,Michael L. Norman
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学科分类Nato Science Series C:
图书封面Titlebook: Astrophysical Radiation Hydrodynamics;  Karl-Heiz A. Winkler,Michael L. Norman Book 1986 D. Reidel Publishing Company, Dordrecht, Holland 1
影响因子This NATO Advanced Research Workshop was devoted to the pre­ sentation, evaluation, and critical discussion of numerical methods in nonrelativistic and relativistic hydrodynamics, radia­ tive transfer, and radiation-coupled hydrodynamics. The unifying theme of the lectures was the successful application of these methods to challenging problems in astrophysics. The workshop was subdivided into 3 somewhat independent topics, each with their own subtheme. Under the heading radiation hydrodynamics were brought together context, theory, methodology, and application of radia­ tive transfer and radiation hydrodynamics in astrophysics. The intimate coupling between astronomy and radiation physics was underscored by examples from past and present research. Frame-dependence of both the equation of transfer (plus moments) and the underlying radiation quantities was discussed and clarified. Limiting regimes in radiation-coupled flow were identified and described; the dynamic diffusion regime received special emphasis. Numerical methods for continuum and line transfer equations in a given background were presented. Two examples of methods for computing dynamically coupled radia­ tion/matter fie
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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
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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
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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)
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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
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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
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