“…To compare the same area covered from multiple observations with different observation geometries and to compare data taken from different instruments, photometric corrections are needed to normalize the reflectance as if it is measured in the same observation geometry. Numerous photometric analyses have been performed on the Moon using the spectral data from ground-based, orbital (i.e., Lunar Orbiter, SMART-1, Kaguya, Chang'E, Chandrayann-1, and LRO itself), and in situ (e.g., the Yutu Rover of the Chang'E-3 lunar mission) observations, covering wavelengths from UV, visible (VIS), and near infrared (NIR; Besse et al, 2013;Buratti et al, 2011;Hapke et al, 2012;Hicks et al, 2011;Hillier et al, 1999;Jin et al, 2015;Kieffer & Stone, 2005;McEwen, 1996;Muinonen et al, 2011;Robinson & Jolliff, 2002;Sato et al, 2014;Wilkman et al, 2014;Wu et al, 2013;Yokota et al, 2011). Notable FUV observations in particular, prior to LRO, have been performed by Apollo-17 Ultraviolet Spectrometer, Hopkins Ultraviolet Telescope, and Galileo-Ultraviolet Spectrometer (Hendrix, 1996;Henry et al, 1995;Lucke et al, 1976).…”