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

DOI10.1007/S11038-016-9485-2zbMath1395.85006OpenAlexW2300611070MaRDI QIDQ1655519

V. Keremidarska, M. Kartalev, M. Dryer

Publication date: 9 August 2018

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s11038-016-9485-2

zbMATH Keywords

comet 67P/C-Gmagnetic cavity boundarymystery regionsingle-fluid modelsolar wind-comet interaction

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20) Radiative transfer in astronomy and astrophysics (85A25)

Cites Work

• Three-dimensional magnetohydrodynamic model of the interaction between the solar wind and cometary atmospheres
• A note on the mass-loaded MHD flow of the solar wind towards a cometary nucleus
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