P13A:
Cassini at Saturn: Science Today and in the Final Three Years II Posters

Monday, 15 December 2014: 1:40 PM-6:00 PM
Chairs:  Linda Joyce Spilker, NASA Jet Propulsion Laboratory, Planetary Science, Pasadena, CA, United States and Donald G Mitchell, JHU/APL, Laurel, MD, United States
Primary Conveners:  Linda Joyce Spilker, NASA Jet Propulsion Laboratory, Planetary Science, Pasadena, CA, United States
Co-conveners:  Scott G Edgington, Jet Propulsion Lab, Pasadena, CA, United States and Nicolas Altobelli, European Space Agency, Villanueva de la Canada, Spain
OSPA Liaisons:  Scott G Edgington, NASA Jet Propulsion Laboratory, Pasadena, CA, United States

Abstracts Submitted to this Session:

 
Modeling plasma pressure anisotropy's effect on Saturn's global magnetospheric dynamics
Matt Tilley1, Erika M Harnett2 and Robert Winglee1, (1)University of Washington, Seattle, WA, United States, (2)University of Washington Seattle Campus, Earth and Space Sciences, Seattle, WA, United States
 
Seasonal and Radial Trends in Saturn’s Thermal Plasma Between the Main Rings and Enceladus
Meredith K Elrod1, Wei-Ling Tseng2, Robert E Johnson3 and Adam Woodson3, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)NTNU National Taiwan Normal University, Department of Earth Sciences, Taipei, Taiwan, (3)Univ Virginia, Charlottesville, VA, United States
 
Field-Aligned Currents in Saturn’s Southern Nightside Magnetosphere: Sub‑Corotation and Planetary Period Oscillation Currents
Gregory James Hunt1, Stanley W H Cowley2, Gabrielle Provan2, Emma J Bunce2, Igor I Alexeev3, Elena Semenovna Belenkaya3, Vladimir V Kalegaev3, Michele Karen Dougherty4 and Andrew J Coates5, (1)University of Leicester, Department of Physics and Astronomy, Leicester, LE1, United Kingdom, (2)University of Leicester, Department of Physics and Astronomy, Leicester, United Kingdom, (3)Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics, Moscow, Russia, (4)Imperial College London, Blackett Laboratory, London, United Kingdom, (5)University College London, Mullard Space Science Laboratory, London, United Kingdom
 
The dynamical properties of E-ring particles derived from CDA impact mass spectra
Rudolfs Namikis1, Mihaly Horanyi2, Frank Postberg3, Ralf Srama3 and Sascha Kempf2, (1)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (2)University of Colorado at Boulder, Physics, Boulder, CO, United States, (3)University of Stuttgart, Stuttgart, Germany
 
The Science from Cassini CIRS, Today and over the Next Three Years
F Michael Flasar, NASA Goddard Space Flight Ctr, Greenbelt, MD, United States
 
The Cassini Imaging Science Subsystem: Science Today and in Cassini's Final Three Years
Robert A West, Jet Propulsion Lab, Pasadena, CA, United States
 
Modeling Saturn's Giant Storms: Water, Ammonia, and the 30-Year Periodicity
Cheng Li and Andrew P. Ingersoll, California Institute of Technology, Pasadena, CA, United States
 
Irregular-Moons Science Today and in Cassini's Final Three Years
Tilmann Denk, Free University of Berlin, Berlin, Germany and Stefano Mottola, German Aerospace Center (DLR), Berlin, Germany
 
SATURN'S INTERNAL MAGNETIC FIELD: EXPECTATIONS FOR CASSINI'S UPCOMING PROXIMAL ORBITS
Marcia E Burton, NASA Jet Propulsion Laboratory, Pasadena, CA, United States and Michele Karen Dougherty, Imperial College London, Blackett Laboratory, London, United Kingdom
 
Magnetic Polarization and Phase Structure of Saturn's 10.7-Hour Oscillations
Japheth Nesta Yates, David J Southwood and Michele Karen Dougherty, Imperial College London, Blackett Laboratory, London, United Kingdom
 
Cassini/MIMI Science Today and Tomorrow
Donald G Mitchell, Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States
 
Energetic Particle Observations from Cassini Deep Tail Passes in 2013-2014
James F Carbary, Johns Hopkins Univ, Laurel, MD, United States, Donald G Mitchell, Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, Norbert Krupp, Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany, Douglas C Hamilton, University of Maryland, College Park, MD, United States and Nick Sergis, National and Kapodistrian University of Athens, Athens, Greece
 
Energetic Neutral Atom (ENA) Movies and Other Cool Data from Cassini's Magnetosphere Imaging Instrument (MIMI)
Martha Bolz Kusterer, Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, Donald G Mitchell, JHU/APL, Laurel, MD, United States, Stamatios M Krimigis, Applied Physics Laboratory Johns Hopkins, Space, Laurel, MD, United States and Jon Duane Vandegriff, Johns Hopkins Univ, Laurel, MD, United States
 
Plasma Speeds Upstream of Saturn and in the Magnetosphere as Measured by Cassini's Magnetospheric Imaging Instrument (MIMI)
Jon Duane Vandegriff1, Matthew E Hill1, George Gloeckler2, Douglas C Hamilton3, Mark Kane4, Stamatios M Krimigis1,5, Donald G Mitchell1, John T Steinberg6, Chihiro Tao7 and Michelle F Thomsen8, (1)JHU/APL, Laurel, MD, United States, (2)Univ Michigan, Ann Arbor, MI, United States, (3)University of Maryland, College Park, MD, United States, (4)Harford Research Institute, Bel Air, MD, United States, (5)Academy of Athens, Office of Space Research and Technology, Athens, Greece, (6)Los Alamos National Lab, Los Alamos, NM, United States, (7)IRAP, Toulouse, France, (8)Planetary Science Institute, Los Alamos, NM, United States
 
GCR as a source for Inner radiation belt of Saturn.
Anna Kotova1, Elias Roussos2, Norbert Krupp2 and Iannis Dandouras3, (1)University Paul Sabatier Toulouse III, Toulouse Cedex 09, France, (2)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (3)IRAP, Toulouse, Italy
 
Geomorphology of Titan's Polar Regions
Samuel P Birch1, Alexander G Hayes Jr1, William E Dietrich2, Michael J Malaska3, Randolph L Kirk4 and Antoine Lucas5, (1)Cornell University, Astronomy, Ithaca, NY, United States, (2)University of California Berkeley, Berkeley, CA, United States, (3)Organization Not Listed, Washington, DC, United States, (4)USGS Grand Canyon Monitoring and Research Center, Flagstaff, AZ, United States, (5)CEA/SACLAY, Paris, France
 
Constraints on Titan rotation from Cassini radar
Bruce G Bills1, Bryan W Stiles1 and Randolph L Kirk2, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)USGS Grand Canyon Monitoring and Research Center, Flagstaff, AZ, United States
 
Rpws Science Today and in Cassini's Final Three Year
Laurent Lamy, Organization Not Listed, Washington, DC, United States
 
UV Imaging Spectroscopy of the Saturn System
Larry W Esposito, Univ of Colorado, Boulder, CO, United States
 
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