Magnetohydrodynamic simulation of a streamer beside a realistic coronal hole |
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| Authors: | S. T. Suess S. T. Wu A. -H. Wang G. Poletto |
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| Affiliation: | (1) Space Science Laboratory, NASA Marshall Space Flight Center, 35812 Huntsville, Alabama, USA;(2) Center for Space Plasma and Aeronomic Research, The University of Alabama in Huntsville, 35899 Huntsville, Alabama;(3) Osservatorio di Arcetri, Firenze, Italy |
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| Abstract: | Existing models of coronal streamers establish their credibility and act as the initial state for transients. The models have produced satisfactory streamer simulations, but unsatisfactory coronal hole simulations. This is a consequence of the character of the models and the boundary conditions. The models all have higher densities in the magnetically open regions than occur in coronal holes (Noci,et al., 1993). |
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| Keywords: | Streamers Coronal Holes MHD Simulations |
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