Simulation of astrophysical phenomena on the basis of high-performance computations

DOI10.1134/S1064562417010185zbMath1368.85004OpenAlexW2606225158MaRDI QIDQ2358600

Yanyan Li

Publication date: 15 June 2017

Published in: Doklady Mathematics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s1064562417010185

zbMATH Keywords

simulationtime discretizationaccretion of interstellar matterastrophysical phenomenacollinear jetsthree-dimensional magnetogasdynamic problems

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Applications to the sciences (65Z05)

Related Items (6)

Kinetic model and magnetogasdynamics equations ⋮ Kinetic algorithms for modeling conductive fluids flow on high-performance computing systems ⋮ Numerical algorithms for systems with extramassive parallelism ⋮ Моделирование задач магнитной гидродинамики на высокопроизводительных вычислительных системах ⋮ A quasi-gasdynamic model for the description of magnetogasdynamic phenomena ⋮ Compact quasi-gas-dynamic system and high performance computing

Cites Work

• Three-level scheme for solving parabolic and elliptic equations
• On an algorithm for solving parabolic and elliptic equations
• Hyperbolic type explicit kinetic scheme of magneto gas dynamics for high performance computing systems
• Kinetic schemes and quasi-gas-dynamic system of equations

This page was built for publication: Simulation of astrophysical phenomena on the basis of high-performance computations