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Fig. A.4
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Fit of our fixed-SHOE Hapke model to the reflectance factor (I/F) as a function of the phase angle for the Cornelia (panels a–f) and Matronalia (g–i) subregions. Panels (a)-(d): Labeled avalanches. Panel (e): Crater floor. Panel (f): Opposite wall. Panel (g): Small crater. Panel (h): Ejecta. Panel (i): Cliff slope.
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