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. 2016 Nov 1;16(11):873–899. doi: 10.1089/ast.2015.1422

FIG. 15.

FIG. 15.

A comparison of reflectance spectra and surface flux spectra using Khare et al. (1984a) and Mahjoub et al. (2012) optical constants, plus a spectrum generated by shifting the Khare constants to match the Archean haze refractive indices measured by Hasenkopf et al. (2010) at 532 nm (called “Khare-Hasenkopf”).