MHD projection of the solar wind structure observed at earth orbit to the sun

Details MHD projection of the solar wind structure observed at earth orbit to the sun MHD projection of the solar wind structure observed at earth orbit to the sun

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ge%26ae..33..153u&link_type=abstract

Geomagnetizm i Aeronomiya (ISSN 0016-7940), vol. 33, no. 3, p. 153-155.

Mathematics

Earth Orbits, Interplanetary Magnetic Fields, Magnetohydrodynamics, Solar Wind Velocity, Space Plasmas, Mathematical Models, Plasma Density, Plasma Pressure, Plasma Temperature

Scientific paper

It is shown that numerical MHD simulation can be used for the inverse projection of actual profiles of solar-wind parameters from earth orbit to a distance of about 0.16 AU. It is shown that the use of numerical MHD models makes it possible to refine the approximation of constant velocity for the inverse projection of velocity structures of the solar wind. It also makes it possible to obtain information on the distribution of interplanetary-plasma parameters (density, pressure, temperature, and magnetic field) to considerably nearer distances to the sun than the earth's orbit.

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