Elivagar Flumina
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Elivagar Flumina is a network of river channels in the region around the Menrva Crater of Titan.[1] Its channels range from being 23 km to 210 km long.[2] The channel system is at least 120 km wide, and it shows signs of erosion.[3] Elivagar Flumina was most likely formed by hydrocarbon flash floods.[1]
References
- 1 2 Williams, David; Radebaugh, Jani; Lopes, Rosaly; Stofan, Ellen (2011). "Geomorphologic mapping of the Menrva region of Titan using Cassini RADAR data". Retrieved 18 June 2016.
- ↑ "Fig. 1. Cassini RADAR image of Menrva and Elivagar Flumina taken during the T3 fly-by, showing the channels near Menrva and the catchment basin (highlighted in blue).". Researchgate. Retrieved 18 June 2016.
- ↑ "ALLUVIAL FANS ON TITAN REVEAL MATERIALS, PROCESSES AND REGIONAL CONDITIONS" (PDF). 2013. Retrieved 18 June 2016.
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