The solar wind current system - Results of numerical calculations

Details The solar wind current system - Results of numerical calculations The solar wind current system - Results of numerical calculations

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26....1p&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, Jan.-Feb. 1986, p. 1-5. In Russian.

Statistics

Computation

Computational Astrophysics, Electric Current, Numerical Analysis, Plasma Currents, Solar Wind Velocity, Current Density, Solar Corona

Scientific paper

Results of numerical calculations of the surface current in the interplanetary current layer and of the volume current in the solar wind for heliocentric distances of 1-10 solar radii are presented. The current intensity is analyzed as a function of the spatial coordinates. It is shown that the three-dimensional current system of the nonaxisymmetric and nonsymmetric (with respect to the helioequator plane) dissipation-free magnetohydrodynamic corona expansion is much more complex than the zonal circular current around the sun, which is the only element of the current system in the spatially symmetric case.

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