Hybrid simulation of space plasmas: models with massless fluid representation of electrons. IV: Kelvin-Helmholtz instability
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Publication:1395126
DOI10.1023/A:1015210812614zbMath1114.76380OpenAlexW282293900MaRDI QIDQ1395126
Publication date: 26 June 2003
Published in: Computational Mathematics and Modeling (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1023/a:1015210812614
Statistical mechanics of plasmas (82D10) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)
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Simulation of space plasma allowing for the Hall effect: magnetic reconnection ⋮ Simulation of space plasma allowing for the Hall effect: Kelvin-Helmholtz and Rayleigh-Taylor instabilities
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