Publication: MNRAS submitted; Authors: P. Judge, P. Bryans, R. Casini, L. Kleint, D. Lacatus, A. Paraschiv, D. Schmit
This paper identifies spectral lines from EUV to infrared wavelengths which are optimally suited to measuring vector magnetic fields as high as possible in the solar atmosphere.
The solar spectrum seen at low resolution, below the atmospheric cutoff at 3100 Angstrom