Simulation of space plasma allowing for the Hall effect: magnetic reconnection
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Publication:851991
DOI10.1007/s10598-005-0026-5zbMath1101.76064OpenAlexW2005356651MaRDI QIDQ851991
Publication date: 27 November 2006
Published in: Computational Mathematics and Modeling (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10598-005-0026-5
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)
Cites Work
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- Hybrid simulation of space plasmas: models with massless fluid representation of electrons. IV: Kelvin-Helmholtz instability
- Hybrid simulation of space plasmas: models with massless fluid representation of electrons. VI: Magnetotail current sheets
- On a plasma sheath separating regions of oppositely directed magnetic field
- Magnetohydrodynamic Equations for Finite Larmor Radius
- Forced magnetic reconnection
- Magnetohydrodynamic equations for systems with large Larmor radius
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