Longitudinal profile data (distance along main stem in meters vs. elevation in meters) for all the valley networks used in the related manuscript 'Did Martian valley networks substantially modify the
Code, movies and climate model outputs for "Gullies on Mars could have formed by melting of water ice during periods of high obliquity" by Dickson et al. Science, 2023.
This dataset contains the materials supporting the study “Origin of Late Noachian-Early Hesperian Valley Networks on Mars: Insights from Landform Evolution and Ice Sheet Modeling.” We include videos
The quadrangle is in the northern Maja Valles region on the west edge of the Chryse Planitia. This map is one in a sequence of three that also includes MTM 15057 and 20057. The sequence covers that pa
