Fig. 1

Dune and plain impact craters on Titan’s surface with (a) VIMS RGB color map background (R:1.59/1.27, G: 2.03/1.27, and B: 1.27/1.08 μm ratios) (Le Mouélic et al. 2019); (b) SAR background (NASA/JPL/Cassini RADAR team); (c) Microwave emissivity map background (Janssen et al. 2016); (d) Titan’s major geomorphological units (Lopes et al. 2020). For (a) and (b), yellow selections correspond to the crater floor, and red selections to the ejecta blanket. The black dashed rectangle in (a) corresponds to the zoomed areas shown in b, c, and d. The Huygens landing site is marked with a white box.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.