Main Objective: Understand the magnetic evolution of coronal holes
Scientific Justification: These observations will support an LWS-funded project to study the effects of high resolution magnetograms (as compared to HMI) on the coronal dynamics in a time-dependent data-driven MHD model. The preferred target is a low latitude coronal hole or polar coronal hole extension near disk center. We need large FOV (40"x60"), high cadence (<12m), and long duration (>4 hours) timeseries of SP scans. The SP data will be inverted using SIR. |
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