МГД моделирование динамики остатка сверхновой с учетом нейтральной компоненты плазмы

DOI10.20948/mm-2022-01-04zbMath1484.76093OpenAlexW4200514975MaRDI QIDQ5023159

Yu. S. Sharova

Publication date: 21 January 2022

Published in: Математическое моделирование (Search for Journal in Brave)

Full work available at URL: http://mathnet.ru/eng/mm4347

zbMATH Keywords

hydrodynamic instabilityinterstellar plasmaHarten-Lax-van Leer contact schemeMARPLE3D software packageradiation-magnetohydrodynamic modelsupernova envelope

Mathematics Subject Classification ID

Finite volume methods applied to problems in fluid mechanics (76M12) Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar dynamics (85A05) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (1)

MARPLE

Uses Software

• HE-E1GODF
• Pluto
• CASTRO
• FLASH

Cites Work

• Unnamed Item
• The piecewise parabolic method (PPM) for gas-dynamical simulations
• A multi-state HLL approximate Riemann solver for ideal magnetohydrodynamics
• Riemann Solvers and Numerical Methods for Fluid Dynamics

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