Numerical simulations of Rayleigh–Taylor and Richtmyer–Meshkov instability using MAH-3 code

Author:

Anuchina N.N.,Volkov V.I.,Gordeychuk V.A.,Es'kov N.S.,Ilyutina O.S.,Kozyrev O.M.

Publisher

Elsevier BV

Subject

Applied Mathematics,Computational Mathematics

Reference25 articles.

1. N.N. Anisimov, V.I. Volkov, A.V. Polionov, Some features of Richtmyer–Meshkov instability evolution, in: Proc. 7IWPCTM, Printing House of RFNC-VNIIEF, Sarov, Russia, 2001, pp. 374–378.

2. N.N. Anuchina, V.I. Volkov, N.S. Es’kov, A method for numerical simulation of contact surface with high distortions, in: Proc. 7IWPCTM, Printing House of RFNC-VNIIEF, Sarov, Russia, 2001, pp. 363–366.

3. 3D numerical simulation of Rayleigh–Taylor instability using MAH-3 code;Anuchina;Laser Particle Beams,2000

4. Numerical simulation of gravitational turbulent mixing;Anuchina;VANT,1982

5. N.N. Anuchina, Yu.A. Kucherenko, V.E. Neuvazhaev et al., Turbulent mixing at the accelerating interface between fluids with different densities, fluid and gas mechanics 6 (1978) 157–160 (in Russian).

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