Upgrades to the Lijiang Coronagraph enable observations showing strong correlations between coronal green-line brightness, magnetic field strength at 1.1 solar radii, and SDO/AIA 21.1 nm emission.
Registration and imaging polarimetry of the Fe 6374 Å red coronal line during the 2017 total solar eclipse.MNRAS2021,503, 5715–5729
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Observational Technological Innovations and Future Development of the Lijiang Coronagraph
Upgrades to the Lijiang Coronagraph enable observations showing strong correlations between coronal green-line brightness, magnetic field strength at 1.1 solar radii, and SDO/AIA 21.1 nm emission.