Astronomy and Astrophysics – Astronomy
Scientific paper
May 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981georl...8..523w&link_type=abstract
Geophysical Research Letters, vol. 8, May 1981, p. 523-526.
Astronomy and Astrophysics
Astronomy
49
Earth Magnetosphere, Geomagnetism, Magnetohydrodynamic Flow, Solar Terrestrial Interactions, Solar Wind, Three Dimensional Flow, Three Dimensional Models, Astronomical Models, Bow Waves, Hydrodynamic Equations, Magnetic Dipoles, Mathematical Models, Shock Wave Propagation
Scientific paper
The results of a global MHD calculation of the steady state solar wind interaction with a dipole magnetic field are presented. The computer code used, being much faster than previous codes, makes it possible to increase the number of grid points in the system by an order of magnitude. The resulting model qualitatively reproduces many of the observed features of the quiet time magnetosphere including the bow shock, magnetopause, and plasma sheet.
Dawson John M.
Walker Ray J.
Wu Congjun
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