Sinuous ridges are exhumed fluvial channel belts formed over millions of years: implications for inverted channels on Mars
Alistair Hayden, California Institute of Technology, Pasadena, CA, United States, Michael P. Lamb, California Institute of Technology, Geological and Planetary Sciences, Pasadena, United States, David C Mohrig, University of Texas at Austin, Department of Earth and Planetary Sciences, Austin, United States, Brandon J McElroy, University of Wyoming, Geology and Geophysics, Laramie, WY, United States, Rebecca M. E. Williams, Planetary Science Institute, Tucson, United States, Paul Myrow, Colorado College, Colorado Springs, CO, United States, Ryan Ewing, Texas A&M, Department of Geology and Geophysics, College Station, United States, Benjamin Thomas Cardenas, Pennsylvania State University Main Campus, Geosciences, University Park, United States and Clyde Pitt Findlay III, Texas A&M University College Station, Department of Geology and Geophysics, College Station, TX, United States
