Turbulent mixing in spherical implosions
作者： David L. Youngs , Robin J. R. Williams
DOI: 10.1002/FLD.1594
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摘要: We discuss the application of numerical code TURMOIL to turbulent mixing in a simple spherical implosion, much simplified version an inertial confinement fusion implosion. Some form Monotone integrated large eddy simulation is required eliminate non-physical oscillations, as shocks and contact discontinuities are present. The dissipation scheme analysed. It argued that this relatively low 'sub-grid' can be precisely quantified. 2007/MOD. Reproduced with permission.
sci-hub.se 参考文章(7)
David J. Benson, Computational methods in Lagrangian and Eulerian hydrocodes Applied Mechanics and Engineering. ,vol. 99, pp. 235- 394 ,(1992) , 10.1016/0045-7825(92)90042-I
David L. Youngs, Three-dimensional numerical simulation of turbulent mixing by Rayleigh-Taylor instability Physics of Fluids. ,vol. 3, pp. 1312- 1320 ,(1991) , 10.1063/1.858059
Hervé Guillard, Angelo Murrone, On the behavior of upwind schemes in the low Mach number limit: II. Godunov type schemes Computers & Fluids. ,vol. 33, pp. 655- 675 ,(2004) , 10.1016/J.COMPFLUID.2003.07.001
D.L. Youngs, Numerical simulation of mixing by Rayleigh-Taylor and Richtmyer-Meshkov instabilities Laser and Particle Beams. ,vol. 12, pp. 725- 750 ,(1994) , 10.1017/S0263034600008557
Dargan M. Frierson, John M. Blondin, Roger A. Chevalier, PULSAR WIND NEBULAE IN EVOLVED SUPERNOVA REMNANTS The Astrophysical Journal. ,vol. 563, pp. 806- 815 ,(2001) , 10.1086/324042
D. L. Youngs, Time-Dependent Multi-Material Flow with Large Fluid Distortion Numerical Methods for Fluid Dynamics. pp. 273- 285 ,(1982)
John M. Blondin, Roger A. Chevalier, Dargan M. Frierson, Pulsar Wind Nebulae in Evolved Supernova Remnants arXiv: Astrophysics. ,(2001) , 10.1086/324042