Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ssrv...52...89b&link_type=abstract
Space Science Reviews (ISSN 0038-6308), vol. 52, Feb. 1990, p. 89-120.
Astronomy and Astrophysics
Astronomy
110
Interstellar Gas, Plasma Interactions, Solar Activity Effects, Solar Wind, Astronomical Models, Solar Corona, Solar Neighborhood
Scientific paper
A survey of the present-day situation in gasdynamical models of solar wind interaction with the local interstellar medium is presented. A role of these models in interpreting a number of observed physical phenomena is investigated. Experimental data and possible observations are considered from the viewpoint of their interpretation on the basis of theoretical models. Attention is concentrated on the main limitations of the gasdynamical models, in particular the two-shock model developed by Baranov et al. (1981 and 1982).
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