Three-dimensional magnetohydrodynamic model of the interaction between the solar wind and cometary atmospheres

DOI10.1134/S0015462815010111zbMath1325.76201OpenAlexW2092221208MaRDI QIDQ893518

D. B. Aleksashov, M. G. Lebedev, V. B. Baranov

Publication date: 19 November 2015

Published in: Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0015462815010111

zbMATH Keywords

solar windMHD flowchuryumov-gerasimenko cometcometary ionosphereHalley comet

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (1)

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

Cites Work

• A multi-state HLL approximate Riemann solver for ideal magnetohydrodynamics

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