Simulation of space plasma allowing for the Hall effect: Kelvin-Helmholtz and Rayleigh-Taylor instabilities

DOI10.1007/S10598-006-0004-6zbMath1100.76070OpenAlexW2018678157MaRDI QIDQ2434025

D. S. Filippychev

Publication date: 31 October 2006

Published in: Computational Mathematics and Modeling (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10598-006-0004-6

Mathematics Subject Classification ID

Interfacial stability and instability in hydrodynamic stability (76E17) Research exposition (monographs, survey articles) pertaining to fluid mechanics (76-02) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Unnamed Item
• High resolution schemes for hyperbolic conservation laws
• Hybrid simulation of space plasmas: models with massless fluid representation of electrons. IV: Kelvin-Helmholtz instability
• Magnetohydrodynamic Equations for Finite Larmor Radius
• Magnetohydrodynamic equations for systems with large Larmor radius
• Stability of the Interface between Two Fluids in Relative Motion

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