Morphometric characteristics of recurring slope lineae initiation and termination points on Mars: elevation, slope, and thermal inertia distinguish RSL-forming sites
Michelle Tebolt1, Sean Corrigan1, Adrian Heath2, Chelsea Jacques1, Patrick Matulka3, Hayley Pearson1, Norbert Schorghofer4, Timothy A Goudge5 and Joseph Levy6, (1)Colgate University, Hamilton, NY, United States, (2)Oregon State University, College of Earth, Ocean, and Atmospheric Sciences, Corvallis, United States, (3)Washington University in St. Louis, St. Louis, MO, United States, (4)University of Hawaii at Manoa, Honolulu, HI, United States, (5)The University of Texas at Austin, Jackson School of Geosciences, Austin, United States, (6)Colgate University, Geology, Hamilton, NY, United States
