Gasdynamic models of physical phenomena occurring in the space. An overview

DOI10.1134/S001546281103001XzbMath1235.76196MaRDI QIDQ408737

V. B. Baranov

Publication date: 11 April 2012

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

zbMATH Keywords

shock wavesheliopausesolar windcharge exchangecometary gascometopauseinterstellar mediumphotoionization

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Research exposition (monographs, survey articles) pertaining to fluid mechanics (76-02) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Research exposition (monographs, survey articles) pertaining to astronomy and astrophysics (85-02)

Cites Work

• Model representations of the interaction between the solar wind and the supersonic interstellar medium flow. Prediction and interpretation of experimental data
• Three-component gas-dynamic model of the interaction of the solar wind with the interstellar medium
• Supersonic solar wind ion flows downstream of the termination shock explained by a two-fluid shock model

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