Flow of an ultra-Alfvenic ideally conducting gas around a superconducting sphere

Details Flow of an ultra-Alfvenic ideally conducting gas around a superconducting sphere Flow of an ultra-Alfvenic ideally conducting gas around a superconducting sphere

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ge%26ae..15..158e&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 15, Jan.-Feb. 1975, p. 158-160.) Geomagnetism and Aeronomy, vol. 15, Aug. 1975, p. 130-132. Tra

Physics

Conducting Fluids, Ideal Gas, Magnetohydrodynamic Flow, Solar Wind, Superconductors, Angular Distribution, Magnetic Fields, Mass Flow Rate, Shock Wave Propagation, Vector Analysis

Scientific paper

The structure of the perturbed solar wind and the forward portion of a streamlined body was studied by Pivovarov (1974) on the basis of a solution to the problem of the flow of the solar wind plasma past a conducting sphere, obtained for the case of parallel mass-velocity and magnetic-field-intensity vectors. The analysis is extended to the case where these vectors are not parallel.

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