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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Bibliographic Details
Published inProgress in earth and planetary science Vol. 3; no. 1
Main Author Inoue, Satoshi
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 04.07.2016
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