“…Several Martian valley systems have undergone extensive aeolian deflation of fine-grained deposits, leaving channels in inverted relief (Williams and Edgett, 2005;Pain et al, 2007;Williams, 2007;Mangold et al, 2008;Newsom et al, 2010). Most of these are fragmentary or exhibit low sinuosity, but an extensive set of inverted sinuous channels is exposed in the Aeolis Dorsa region, centered at about 5°S and 150°E (Burr et al, 2009(Burr et al, , 2010Williams et al, 2009Williams et al, , 2013 (Fig.…”