P13B
Titan: Understanding Saturn's Mysterious Moon II Posters

Monday, 14 December 2015: 13:40-18:00
Poster Hall (Moscone South)
Primary Conveners:  Robert M. Nelson, Planetary Science Institute, Pasadena, CA, United States
Conveners:  Rosaly M C Lopes, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and Joseph H Westlake, JHUAPL, Laurel, MD, United States
Chairs:  Robert M. Nelson, Planetary Science Institute, Pasadena, CA, United States, Rosaly M C Lopes, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and Joseph H Westlake, JHUAPL, Laurel, MD, United States
OSPA Liaisons:  Rosaly M C Lopes, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
 
Identification of Acetylene on Titan's Surface (61547)
Sandeep Singh1, Thomas B McCord2, Sebastien Rodriguez3, Jean Philippe Combe2, Thomas Cornet4, Stephane Le Mouelic5, Luca Maltagliati6, Vincent Chevrier1 and Roger Nelson Clark7, (1)University of Arkansas, Fayetteville, AR, United States, (2)Bear Fight Institute, Winthrop, WA, United States, (3)AIM - CEA/CNRS/Uni. P7, Gif/Yvette, France, (4)European Space Agency, Villanueva De La Can, Spain, (5)CNRS, Paris Cedex 16, France, (6)Paris Observatory Meudon, Meudon, France, (7)Planetary Science Institute Tucson, Tucson, AZ, United States
 
Onset and Cessation of Thermal Convection within Titan’s Ice Shell (62234)
Giuseppe Mitri1, Gabriel Tobie1 and Gael Choblet2, (1)University of Nantes, Nantes, France, (2)LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France
 
Changes on Titan’s surface (62790)
Anezina Solomonidou1,2, Rosaly M C Lopes1, Athena Coustenis2, Michael J Malaska3, Christophe Sotin1, Sebastien Rodriguez4, Michael A Janssen5, Pierre Drossart6, Kenneth J Lawrence1, Christos k Matsoukas7, Mathieu Hirtzig8, Stephane Le Mouelic9, Ralf Jaumann10, Robert Hamilton Brown11 and Emmanuel Bratsolis12, (1)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)Paris Observatory Meudon, Meudon, France, (3)Organization Not Listed, Washington, DC, United States, (4)AIM - CEA/CNRS/Uni. P7, Gif/Yvette, France, (5)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (6)LESIA Observatoire de Paris, Meudon, France, (7)National and Kapodistrian University of Athens, Athens, Greece, (8)Fondation “La main à la pâte”, Montrouge, France, (9)CNRS, Paris Cedex 16, France, (10)German Aerospace Center DLR Berlin, Berlin, Germany, (11)University of Arizona, Tucson, AZ, United States, (12)National and Kapodistrian University of Athens, Department of Physics, Athens, Greece
 
Nature, Distribution, and Origin of Titan’s Undifferentiated Plains (“Blandlands”) (62958)
Rosaly M C Lopes1, Michael J Malaska2, Anezina Solomonidou1, Alice Anne Le Gall3, Michael A Janssen4, Catherine Neish5, Elizabeth P Turtle6, Samuel P Birch7, Alexander Hayes8, Jani Radebaugh9, Athena Coustenis10, Bryan W Stiles4, Randolph L Kirk11, Karl L Mitchell4, Kenneth J Lawrence1 and Cassini RADAR Team, (1)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)Organization Not Listed, Washington, DC, United States, (3)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)Florida Institute of Technology, Melbourne, FL, United States, (6)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (7)University of California Berkeley, Berkeley, CA, United States, (8)Cornell University, Department of Astronomy, Ithaca, NY, United States, (9)Brigham Young University, Provo, UT, United States, (10)Paris Observatory Meudon, Meudon, France, (11)USGS Grand Canyon Monitoring and Research Center, Flagstaff, AZ, United States
 
Dark Areas on Equatorial Regions of Titan: Implication in Particles Size of Water-Ice and Combination with Tholins. (63236)
Jeremy Florian Brossier1,2, Katrin Stephan1,2 and Ralf Jaumann2, (1)German Aerospace Center DLR Berlin, Berlin, Germany, (2)DLR - German Aerospace Center, Institute of Planetary Research, Berlin, Germany
 
Variations in Titan’s Ionospheric Densities over a 10 Year Time Period of the Cassini Mission (65069)
Hadi Madanian, University of Kansas, Lawrence, KS, United States
 
Simultaneous Cartography of Aerosol Opacity and Surface Albedo of Titan by the Massive Inversion of the Cassini/VIMS Dataset (69084)
Luca Maltagliati1, Sebastien Rodriguez2, Christophe Sotin3, Pascal Rannou4, Thomas Cornet5, Mathieu Hirtzig6, Thomas Appéré2, Anezina Solomonidou3, Stephane Le Mouelic7, Athena Coustenis8 and Robert Hamilton Brown9, (1)CEA Commissariat à l'Energie Atomique Saclay, Gif-Sur-Yvette Cedex, France, (2)AIM - CEA/CNRS/Uni. P7, Gif/Yvette, France, (3)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (4)GSMA - University of Reims Champagne-Ardennes, Reims, France, (5)European Space Agency, Villanueva De La Can, Spain, (6)Fondation “La main à la pâte”, Montrouge, France, (7)CNRS, Paris Cedex 16, France, (8)Paris Observatory Meudon, Meudon, France, (9)University of Arizona, Tucson, AZ, United States
 
Spectral detection of complex organics in the hydrocarbon lakes of Titan (69184)
Delphine Nna-Mvondo, CNRS, Laboratoire de Planétologie et Géodynamique, Nantes, France
 
Backscatter modelling and inversion from Cassini/SAR data: Implications for Titan’s sand seas properties and climatic conditions (69326)
Antoine Lucas1, Sebastien Rodriguez1, Florentin Lemonnier1, Philippe Paillou2, Alice Anne Le Gall3 and Clement Narteau4, (1)AIM - CEA/CNRS/Uni. P7, Gif/Yvette, France, (2)University of Bordeaux 1, Talence, France, (3)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (4)Institut de Physique du Globe de Paris, Paris, France
 
A RT-based Technique for the Analysis and the Removal of Titan's Atmosphere by Cassini/VIMS-IR data (69830)
Giuseppe Sindoni1, Federico Tosi1, Alberto Adriani1, Maria Luisa Moriconi2, Emiliano D'Aversa1, Davide Grassi1, Fabrizio Oliva1, Bianca Maria Dinelli2 and Elisa Castelli2, (1)IAPS-INAF, Rome, Italy, (2)CNR Institute of Atmospheric Sciences and Climate, Bologna, Italy
 
Computing Global Mosaics of Titan With the VIMS Imaging Spectrometer (71972)
Stephane Le Mouelic1, Thomas Cornet2, Sebastien Rodriguez3, Christophe Sotin4, Jason W Barnes5, Robert Hamilton Brown6, Kevin H Baines7, Bonnie J Buratti4, Roger Nelson Clark8 and Philip D Nicholson9, (1)CNRS, Paris Cedex 16, France, (2)European Space Agency, Villanueva De La Can, Spain, (3)AIM - CEA/CNRS/Uni. P7, Gif/Yvette, France, (4)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (5)University of Idaho, Moscow, ID, United States, (6)University of Arizona, Tucson, AZ, United States, (7)Jet Propulsion Laboratory, Pasadena, CA, United States, (8)Planetary Science Institute Tucson, Tucson, AZ, United States, (9)Cornell University, Ithaca, NY, United States
 
Geomorphology of Titan's polar terrains: Using the landscape’s topographic form to constrain surface processes (72906)
Samuel P Birch, University of California Berkeley, Berkeley, CA, United States
 
Topographic Constraints on the Evolution and Connectivity of Titan's Lacustrine Basins (73619)
Alexander G Hayes Jr, Cornell University, Astronomy, Ithaca, NY, United States
 
Examining the exobase approximation: DSMC models of Titan’s upper atmosphere (73761)
Orenthal James Tucker, University of Michigan Ann Arbor, Ann Arbor, MI, United States
 
Kinematic model of Titan’s rotation from Cassini radar data (75012)
Bruce G Bills1, Bryan W Stiles1, Alexander Hayes2 and Sam Birch2, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Cornell University, Department of Astronomy, Ithaca, NY, United States
 
Mulitple Origins of Sand Dune-Topography Interactions on Titan (76477)
Holly Goggin, Texas A & M University College Station, College Station, TX, United States, Ryan C Ewing, Texas A&M University, College Station, TX, United States, Alexander Hayes, Cornell University, Department of Astronomy, Ithaca, NY, United States and Julia Cisneros, Texas A & M University, College Station, TX, United States
 
CRYOCHEM modeling of Titan’s liquid: the effects of hydrogen cyanide (HCN) (76580)
Sugata P Tan, Planetary Science Institute Tucson, Tucson, AZ, United States, Jeffrey S Kargel, University of Arizona, Tucson, AZ, United States, Hertanto Adidharma, University of Wyoming, Laramie, WY, United States and Giles M Marion, DEES DRI, Reno, NV, United States
 
Dissolution on Titan and on Earth: Towards the Age of Titan's Karstic-like Landscapes (78066)
Thomas Cornet, European Space Agency, Villanueva De La Can, Spain, Daniel Cordier, Institut UTINAM CNRS INSU, Univ. Franche Comte, Besancon, France, Tangui Le Bahers, Universite de Lyon 1, ENS-Lyon, Lyon, France, Olivier Bourgeois, Universite de Nantes - CNRS, Nantes, France, Cyril Fleurant, LETG UMR CNRS 6554 Universite d'Angers, Angers, France, Stephane Le Mouelic, CNRS, Paris Cedex 16, France and Nicolas Altobelli, European Space Agency, Villanueva de la Canada, Spain
 
Long-Lived Storms and Squall Lines on Titan (79203)
Scot CR Rafkin, Southwest Research Institute Boulder, Boulder, CO, United States
 
An Overview of the Bathymetry and Composition of Titan’s Hydrocarbon Seas from the Cassini RADAR Altimeter (79777)
Marco Mastrogiuseppe, Sapienza University of Rome, Rome, Italy
 
Carbon Dioxide Chemistry on Titan’s Surface (79801)
Robert P Hodyss1, Morgan L Cable2, Michael J Malaska3 and Tuan Hoang Vu2, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Organization Not Listed, Washington, DC, United States
 
Compositional and Optical Properties of Titan Haze Analogs Using Aerosol Mass Spectrometry, Photoacoustic Spectroscopy and Cavity Ring-Down Spectroscopy (83542)
Melissa Ugelow, Cooperative Institute for Research in Environmental Sciences, Boulder, CO, United States
 
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