CRASH: A BLOCK-ADAPTIVE-MESH CODE FOR RADIATIVE SHOCK HYDRODYNAMICS-IMPLEMENTATION AND VERIFICATION
Abstract
We describe the Center for Radiative Shock Hydrodynamics (CRASH) code, a block-adaptive-mesh code for multi-material radiation hydrodynamics. The implementation solves the radiation diffusion model with a gray or multi-group method and uses a flux-limited diffusion approximation to recover the free-streaming limit. Electrons and ions are allowed to have different temperatures and we include flux-limited electron heat conduction. The radiation hydrodynamic equations are solved in the Eulerian frame by means of a conservative finite-volume discretization in either one-, two-, or three-dimensional slab geometry or in two-dimensional cylindrical symmetry. An operator-split method is used to solve these equations in three substeps: (1) an explicit step of a shock-capturing hydrodynamic solver; (2) a linear advection of the radiation in frequency-logarithm space; and (3) an implicit solution of the stiff radiation diffusion, heat conduction, and energy exchange. We present a suite of verification test problems to demonstrate the accuracy and performance of the algorithms. The applications are for astrophysics and laboratory astrophysics. The CRASH code is an extension of the Block-Adaptive Tree Solarwind Roe Upwind Scheme (BATS-R-US) code with a new radiation transfer and heat conduction library and equation-of-state and multi-group opacity solvers. Both CRASH and BATS-R-US are part of the publicly available Spacemore »
- Authors:
-
- Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109 (United States)
- Department of Aerospace Engineering, University of Michigan, Ann Arbor, MI 48109 (United States)
- Nuclear Engineering and Radiological Sciences, University of Michigan, Ann Arbor, MI 48109 (United States)
- Computer Science and Engineering, University of Michigan, Ann Arbor, MI 48109 (United States)
- Department of Nuclear Engineering, Texas A and M University, College Station, TX 77843 (United States)
- Department of Mathematics, University of Michigan, Ann Arbor, MI 48109 (United States)
- Publication Date:
- OSTI Identifier:
- 21560382
- Resource Type:
- Journal Article
- Journal Name:
- Astrophysical Journal, Supplement Series
- Additional Journal Information:
- Journal Volume: 194; Journal Issue: 2; Other Information: DOI: 10.1088/0067-0049/194/2/23; Journal ID: ISSN 0067-0049
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ALGORITHMS; ASTROPHYSICS; DIFFUSION; ELECTRONS; HYDRODYNAMICS; IMPLEMENTATION; RADIANT HEAT TRANSFER; THERMAL CONDUCTION; VERIFICATION; ELEMENTARY PARTICLES; ENERGY TRANSFER; FERMIONS; FLUID MECHANICS; HEAT TRANSFER; LEPTONS; MATHEMATICAL LOGIC; MECHANICS; PHYSICS
Citation Formats
Van der Holst, B, Toth, G, Sokolov, I V, Myra, E S, Fryxell, B, Drake, R P, Powell, K G, Holloway, J P, Stout, Q, Adams, M L, Morel, J E, and Karni, S. CRASH: A BLOCK-ADAPTIVE-MESH CODE FOR RADIATIVE SHOCK HYDRODYNAMICS-IMPLEMENTATION AND VERIFICATION. United States: N. p., 2011.
Web. doi:10.1088/0067-0049/194/2/23.
Van der Holst, B, Toth, G, Sokolov, I V, Myra, E S, Fryxell, B, Drake, R P, Powell, K G, Holloway, J P, Stout, Q, Adams, M L, Morel, J E, & Karni, S. CRASH: A BLOCK-ADAPTIVE-MESH CODE FOR RADIATIVE SHOCK HYDRODYNAMICS-IMPLEMENTATION AND VERIFICATION. United States. https://doi.org/10.1088/0067-0049/194/2/23
Van der Holst, B, Toth, G, Sokolov, I V, Myra, E S, Fryxell, B, Drake, R P, Powell, K G, Holloway, J P, Stout, Q, Adams, M L, Morel, J E, and Karni, S. 2011.
"CRASH: A BLOCK-ADAPTIVE-MESH CODE FOR RADIATIVE SHOCK HYDRODYNAMICS-IMPLEMENTATION AND VERIFICATION". United States. https://doi.org/10.1088/0067-0049/194/2/23.
@article{osti_21560382,
title = {CRASH: A BLOCK-ADAPTIVE-MESH CODE FOR RADIATIVE SHOCK HYDRODYNAMICS-IMPLEMENTATION AND VERIFICATION},
author = {Van der Holst, B and Toth, G and Sokolov, I V and Myra, E S and Fryxell, B and Drake, R P and Powell, K G and Holloway, J P and Stout, Q and Adams, M L and Morel, J E and Karni, S},
abstractNote = {We describe the Center for Radiative Shock Hydrodynamics (CRASH) code, a block-adaptive-mesh code for multi-material radiation hydrodynamics. The implementation solves the radiation diffusion model with a gray or multi-group method and uses a flux-limited diffusion approximation to recover the free-streaming limit. Electrons and ions are allowed to have different temperatures and we include flux-limited electron heat conduction. The radiation hydrodynamic equations are solved in the Eulerian frame by means of a conservative finite-volume discretization in either one-, two-, or three-dimensional slab geometry or in two-dimensional cylindrical symmetry. An operator-split method is used to solve these equations in three substeps: (1) an explicit step of a shock-capturing hydrodynamic solver; (2) a linear advection of the radiation in frequency-logarithm space; and (3) an implicit solution of the stiff radiation diffusion, heat conduction, and energy exchange. We present a suite of verification test problems to demonstrate the accuracy and performance of the algorithms. The applications are for astrophysics and laboratory astrophysics. The CRASH code is an extension of the Block-Adaptive Tree Solarwind Roe Upwind Scheme (BATS-R-US) code with a new radiation transfer and heat conduction library and equation-of-state and multi-group opacity solvers. Both CRASH and BATS-R-US are part of the publicly available Space Weather Modeling Framework.},
doi = {10.1088/0067-0049/194/2/23},
url = {https://www.osti.gov/biblio/21560382},
journal = {Astrophysical Journal, Supplement Series},
issn = {0067-0049},
number = 2,
volume = 194,
place = {United States},
year = {Wed Jun 01 00:00:00 EDT 2011},
month = {Wed Jun 01 00:00:00 EDT 2011}
}