Model representations of the interaction between the solar wind and the supersonic interstellar medium flow. Prediction and interpretation of experimental data

DOI10.1007/S10697-006-0089-9zbMath1200.76227OpenAlexW1964243384MaRDI QIDQ605768

V. B. Baranov, V. V. Izmodenov

Publication date: 25 November 2010

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

Full work available at URL: https://doi.org/10.1007/s10697-006-0089-9

zbMATH Keywords

Monte Carlo methodshock waveheliopausesolar windheliospheric interfacekinetic-gasdynamic modellocal interstellar mediumresonance charge-exchange

Mathematics Subject Classification ID

Experimental work for problems pertaining to fluid mechanics (76-05) Supersonic flows (76J20) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Experimental work for problems pertaining to astronomy and astrophysics (85-05)

Related Items (3)

Gasdynamic models of physical phenomena occurring in the space. An overview ⋮ Comparison of the Eulerian and Lagrangian approaches to studying the peculiarities of the interstellar dust distribution in the heliosphere in the framework of the cold gas model ⋮ Interaction of the supersonic stellar wind with free stream of the interstellar medium: the effect of the azimuthal magnetic field of the star

Cites Work

• Three-component gas-dynamic model of the interaction of the solar wind with the interstellar medium
• Solar cycle influence on the interaction of the solar wind with Local Interstellar Cloud

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