“…The derived total, fine-, and coarse-dust backscatter coefficients β d , β df , and β dc are then converted to respective dust extinction values σ d , σ df , and σ dc by means of appropriate dust extinction-to-backscatter ratios or lidar ratios S d , S df , and S dc . As shown in Table 2, the 532 nm dust lidar ratio S d may vary from about 30 to 60 sr for different mineral dust types (Müller et al, 2007;Tesche et al, 2011;Mamouri et al, 2013;Nisantzi et al, 2015;Groß et al, 2015;Veselovskii et al, 2016;Haarig et al, 2017;Hofer et al, 2017;Shin et al, 2018). However, for most dust regions, except the western Sahara, the typical dust lidar ratio is 40 sr at 532 nm.…”