Investigation of the Middle Corona with SWAP and a Data-Driven Non-Potential Coronal Magnetic Field Model.
Karen A MeyerDuncan H MackayDana-Camelia TalpeanuLisa A UptonMatthew J WestPublished in: Solar physics (2020)
The online version of this article (10.1007/s11207-020-01668-2) contains supplementary material, which is available to authorized users.