Magnetic flux transport by turbulent reconnection in astrophysical flows

DOI10.1088/0031-8949/86/01/018401zbMath1272.85008arXiv1112.4871OpenAlexW2011062603MaRDI QIDQ2844884

R. Santos-Lima, M. R. M. Leão, G. A. Guerrero, G. Kowal, Elisabete M de Gouveia Dal Pino, Alexander Lazarian

Publication date: 20 August 2013

Published in: Physica Scripta (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1112.4871

zbMATH Keywords

MHDturbulencemagnetohydrodynamicsturbulent reconnectionstar formationastrophysical flowsaccretion discdynamo processesmagnetic flux transport

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Electromagnetic theory (general) (78A25) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Stability and instability of geophysical and astrophysical flows (76E20)

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