C. Daudon
YOU?
Author Swipe
View article: Inferring Discharge From River Geometry on Titan
Inferring Discharge From River Geometry on Titan Open
Titan's dense atmosphere, composed mainly of methane and nitrogen, maintains a methane cycle that shapes its surface. Like water on Earth, methane precipitation erodes Titan's surface, carving river networks at all latitudes, as revealed b…
View article: Inferring wind speed from ripple and dune migration on Mars
Inferring wind speed from ripple and dune migration on Mars Open
Dunes and ripples are markers of eolian activity. Dunes arise and evolve from the action of wind blowing on sand grains and can thus provide information on past and current wind regime. They constantly adjust and adapt their shape through …
View article: Rivers as witnesses of Titan's latitudinal climate variability
Rivers as witnesses of Titan's latitudinal climate variability Open
Titan's rich and dense atmosphere, composed mainly of methane and nitrogen, maintains a methane cycle that shapes its surface, like the water cycle on Earth. Methane precipitations erodes Titan's surface and forms complex river networks ob…
View article: A New Digital Terrain Model of the Huygens Landing Site on Saturn's Largest Moon, Titan
A New Digital Terrain Model of the Huygens Landing Site on Saturn's Largest Moon, Titan Open
River valleys have been observed on Titan at all latitudes by the Cassini‐Huygens mission. Just like water on Earth, liquid methane carves into the substrate to form a complex network of rivers, particularly stunning in the images acquired…