MHD simulation of the inner-heliospheric magnetic field
Author:
Affiliation:
1. Institut für Theoretische Physik IV; Ruhr-Universität Bochum; Bochum Germany
2. Max-Planck-Institut für Sonnensystemforschung; Katlenburg-Lindau Germany
3. Institut für Astro-und Teilchenphysik; Universität Innsbruck; Innsbruck Austria
Funder
Deutsche Forschungsgemeinschaft (DFG)
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Reference58 articles.
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3. Improved Method for Specifying Solar Wind Speed Near the Sun
4. Weber and Davis revisited - mass losing rotating magnetic winds;Barker;Astrophys. J.,1982
5. The three-dimensional structure of magnetostatic atmospheres. II - modeling the large-scale corona;Bogdan;Astrophys. J.,1986
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