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A note on the mass-loaded MHD flow of the solar wind towards a cometary nucleus

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Publication:1180210
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DOI10.1007/BF00646450zbMath0736.76079MaRDI QIDQ1180210

K. R. Flammer, D. A. Mendis

Publication date: 27 June 1992

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


zbMATH Keywords

conditions at infinityconservation equations1-dimensional steady state, mass accreting \(MHD\) flowFaradays lawself-reversal


Mathematics Subject Classification ID

Ionized gas flow in electromagnetic fields; plasmic flow (76X05)


Related Items (1)

Revisiting the single-fluid modeling of the solar wind-comet interaction: closer look at the cometosheath







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