Fig. 7
Scatter plots of integrated intensities over the SWAP coronal features against the respective HMI magnetic flux density. HMI eAR vs., SWAP eAR, HMI CH vs. SWAP CH, HMI QS vs. SWAP QS, and HMI full-disk vs. SWAP full-disk are shown here. The lowest panel shows the HMI full-disk magnetic density vs. the LYRA aluminium channel and vs. the daily sunspot number. The data period spans from 1 January 2011 until 1 January 2016.
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