Self consistent MHD modeling of the solar wind from coronal holes with distinct geometries

Details Self consistent MHD modeling of the solar wind from coronal holes with distinct geometries Self consistent MHD modeling of the solar wind from coronal holes with distinct geometries

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...65s&link_type=abstract

Universidad Nacional Autonoma de Mexico, International Solar Wind 8 Conference, p. 65

Physics

Solar Wind, Magnetohydrodynamic Flow, Solar Corona, Coronal Holes, Solar Activity Effects, Flow Characteristics, Symmetry, Models, Iterative Solution

Scientific paper

Utilizing an iterative scheme, a self-consistent axisymmetric MHD model for the solar wind has been developed. We use this model to evaluate the properties of the solar wind issuing from the open polar coronal hole regions of the Sun, during solar minimum. We explore the variation of solar wind parameters across the extent of the hole and we investigate how these variations are affected by the geometry of the hole and the strength of the field at the coronal base.

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