A hydromagnetic model of corotating conductive solar wind streams

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DOI10.1007/BF00651414zbMath0582.76050OpenAlexW2017913668MaRDI QIDQ1068631

Publication date: 1984

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00651414

zbMATH Keywords

invariants approximate solution algebraic method magnetic flux admissible solution entropy equation angular momentum efflux corotating solar wind stream energy efflux interplanetary condition mass efflux quasi-azimuthal symmetry steady hydromagnetic flow thermally conductive flux tube vanishing pressure at infinity

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

An inviscid model of the solar wind

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