The EUV spectrum of the Sun is not the same in all visible structures, e.g. the active region corona is typically hotter than the quiet Sun corona. The spatial resolution of the SERTS spectrograph allows us to obtain distinct spectra for individual solar features. Calibrated emission line catalogs are presented below for active, quiet and off-limb coronal emission. In the 1989 linelist the linewidths quoted represent observed widths. In all other tables the instrument profile was subtracted and the linewidths quoted represent actual solar widths.
Active Region Data
Quiet Sun Data
Solar Limb Data
Last Revised: Wednesday, 29-Nov-2006 07:36:52 EST
Responsible NASA Official: joseph.davila@gsfc.nasa.gov
NASA iT Security Banner & Privacy Statement
Feedback and comments: Emilie Drobnes (curator)