Gasdynamic structure of the heliosphere - Theory and experiment

Details Gasdynamic structure of the heliosphere - Theory and experiment Gasdynamic structure of the heliosphere - Theory and experiment

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roimz...3....3b&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Mekhanika Zhidkosti i Gaza (ISSN 0568-5281), no. 3, p. 3-24.

Mathematics

Gas Dynamics, Heliosphere, Interstellar Gas, Solar Wind, Supersonic Flow, Interplanetary Magnetic Fields, Mathematical Models, Monte Carlo Method

Scientific paper

The development of gasdynamic models of the structure of the heliosphere is reviewed from a historical perspective. A gasdynamic model of supersonic flow of interstellar gas past solar wind is described. Attention is then given to current scientific programs concerned with the study of the circumsolar space at large heliocentric distances. Some new gasdynamic problems associated with these programs are formulated.

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