Fig. 10
From: Cold-based glaciation of Pavonis Mons, Mars: evidence for moraine deposition during glacial advance
Model results depicting changes in the ice extent and ice deposit properties in the distal portion of the simulated ice deposit. Ice thickness (a), basal ice temperature (b), and ice surface flow velocity (c) are indicated by the colored contours plotted against the distance along the flowline shown in Fig. 6 (left y-axis) and time (x-axis). White regions in these panels contain no ice. The gray region in (c) indicates that ice is present, but the surface flow velocity less than 10− 5 m/year. The black line in each panel gives the obliquity history over this time period according to the right y-axis with blue filled sections indicating times of ice accumulation in headward section of the simulated flowline