Physics – Geophysics
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.confr..65p&link_type=abstract
Institute of Applied Geophysics, International Solar Wind 8 Conference, p. 65
Physics
Geophysics
Solar Corona, Solar Rotation, Solar Wind, Electric Fields, Field Aligned Currents, Polar Regions, Magnetohydrodynamic Flow, Relativity, Earth Magnetosphere, Three Dimensional Models, Electric Current
Scientific paper
The calculation of the solar rotation electro-dynamical effects in the near-the-Sun solar wind seems more convenient from the non-inertial corotating reference frame. This implies some modification of the 3-D MHD equations generally on the base of the General Theory of Relativity. The paper deals with the search of stationary (in corotating non-inertial reference frame) solutions of the modified 3-D MHD equations for the in near-the-Sun high latitude sub-alfvenic solar wind. The solution is obtained requiring electric fields and field-aligned electric currents in the high latitude near-the-Sun solar wind. Various scenario are explored self-consistently via a number of numerical experiments. The analogy with the high latitude Earth's magnetosphere is used for the interpretation of the results. Possible observational manifestations are discussed.
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