Mapping of Solar Magnetic Fields from the Photosphere to the Top of the Chromosphere with CLASP2
Coronal heating, chromospheric heating, and the heating & acceleration of the solar wind, are well-known problems in solar physics. Additionally, knowledge of the magnetic energy that powers solar flares and coronal mass ejections, important drivers of space weather, is handicapped by imperfect determination of the magnetic field in the sun's
McKenzie, D. et al.
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2021