“…In addition, a series of post processing procedures have been developed aiming at the improvement of the spectral solar UV measurements' accuracy. These, include methods for correcting the measurements for angular response errors (Seckmeyer and Bernhard, 1993;Bais et al, 1998;Feister et al, 1996), for wavelength scale errors (Huber et al, 1993;Slaper et al, 1995;Slaper and Koskela, 1997), for temperature dependence (Weatherhead et al, 2001;Capellani and Kochler, 1999), for stray light rejection (Davies, 1996;Bais et al, 1997a) and for spikes (Meinander et al, 2003).…”