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.
The Structure of Coronal Mass Ejections Recorded by the K-Coronagraph at Mauna Loa Solar Observatory.ApJ Lett.2023,952, L22–L28
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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.