Magnetohydrodynamics modeling of coronal magnetic field and solar eruptions based on the photospheric magnetic field
In this paper, we summarize current progress on using the observed magnetic fields for magnetohydrodynamics (MHD) modeling of the coronal magnetic field and of solar eruptions, including solar flares and coronal mass ejections (CMEs). Unfortunately, even with the existing state-of-the-art solar phys...
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Published in | Progress in earth and planetary science Vol. 3; no. 1 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
Berlin/Heidelberg
Springer Berlin Heidelberg
04.07.2016
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Subjects | |
Online Access | Get full text |
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