California Institute of Technology, Pasadena, CA, United States; European Space Astronomy Centre, European Space Agency, Madrid, Spain; LESIA-Observatoire de Paris, Paris Sciences and Letters Research University, CNRS, Sorbonne Université, Université Paris-Diderot, Meudon, France; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States; Institut de Physique du Globe de Paris, CNRS-UMR 7154, Université Paris-Diderot, USPC, Paris, France; Institut de Planétologie et d'Astrophysique de Grenoble, Université Grenoble Alpes, CNRS, Grenoble, France; Fondation “La main à la pâte”, Montrouge, France; Department of Physics, University of Athens, Athens, Greece; Department of Geological Sciences, Brigham Young University, Provo, UT, United States; Institute of Planetary Research, DLR, Berlin, Germany; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, United States; Laboratoire de Planétologie et Géodynamique, CNRS UMR 6112, Université de Nantes, Nantes, France; LATMOS/IPSL, UPMC Université Paris 6, Sorbonne Universités, UVSQ, CNRS, Paris, France; European Space Research and Technology Centre, European Space Agency, Noordwijk, Netherlands; KTH-Royal Institute of Technology, Stockholm, Sweden; Department of Earth, Planetary, and Space Sciences, University of Calilfornia, Los Angeles, CA, United States
Recommended Citation:
Solomonidou A.,Coustenis A.,Lopes R.M.C.,et al. The Spectral Nature of Titan's Major Geomorphological Units: Constraints on Surface Composition[J]. Journal of Geophysical Research: Planets,2018-01-01,123(2)