Example of the numerical calculation of the three-dimensional structure of the solar wind

Details Example of the numerical calculation of the three-dimensional structure of the solar wind Example of the numerical calculation of the three-dimensional structure of the solar wind

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..371p&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, May-June 1985, p. 371-376. In Russian.

Statistics

Computation

4

Computational Fluid Dynamics, Current Sheets, Interplanetary Magnetic Fields, Solar Wind Velocity, Three Dimensional Flow, Coronal Loops, Free Boundaries, Radial Velocity

Scientific paper

The steady three-dimensional flow of the solar wind in the corona and in the presence of a ribbon of coronal loops, arcades, and helmet-shaped rays is considered. The model used is that of Meier flow from two solar 'nozzles' with an interplanetary current sheet as the free boundary, separating the influence regions of the nozzles. A four-sector structure of the solar wind is obtained, with a high-velocity stream in each sector.

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