P41B
Jove You Inside Out: Giant Planet Interiors, Atmospheres, Aurorae, and Ionospheres II Posters

Thursday, 17 December 2015: 08:00-12:20
Poster Hall (Moscone South)
Primary Conveners:  Kunio M Sayanagi, Hampton University, Hampton, VA, United States
Conveners:  Ulyana Dyudina, Caltech, Pasadena, CA, United States, Scott G Edgington, NASA Jet Propulsion Laboratory, Pasadena, CA, United States and Padma A Yanamandra-Fisher, Space Science Institute Rancho Cucamonga, Rancho Cucamonga, CA, United States
Chairs:  Ravit Helled, Tel-Aviv University, Tel Aviv, Israel and Scott G Edgington, NASA Jet Propulsion Laboratory, Pasadena, CA, United States
OSPA Liaisons:  Morgan E O'Neill, Weizmann Institute of Science, Rehovot, Israel
 
Neptune’s Vertical Wind Shear Modeled with a Generalized Thermal Wind Equation  (61968)
Joshua Tollefson, University of California Berkeley, Berkeley, CA, United States
 
An abrupt change in the long-term cooling of the ionosphere of Uranus (77927)
Henrik Melin, University of Leicester, Leicester, LE1, United Kingdom
 
HST and ground-based observations of bright storms on Uranus during 2014-2015. (65742)
Kunio M Sayanagi, Hampton University, Hampton, VA, United States
 
Photochemistry in Saturn’s Ring-Shadowed Atmosphere: Modulation of Hydrocarbons and Observations of Dust Content (77619)
Scott G Edgington1, Sushil K Atreya2, Eric H Wilson3, Kevin H Baines4, Robert A West1, Gordon L Bjoraker5, Leigh N. Fletcher6 and Thomas Momary7, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (3)Space Environment Technologies, Pacific Palisades, CA, United States, (4)Jet Propulsion Laboratory, Pasadena, CA, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)University of Leicester, Leicester, United Kingdom, (7)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
 
Peeking into Saturn's Atmosphere: the HST Low-Phase Angle View (66186)
Santiago Perez-Hoyos1, Jose Francisco Sanz-Requena2, Agustin Sanchez-Lavega1, Ricardo Hueso3, Teresa del Rio-Gaztelurrutia1, Jose F Rojas1, Amy A Simon4, Michael H Wong5, Imke De Pater5 and Patrick GJ Irwin6, (1)University of the Basque Country, Donostia, Spain, (2)Universidad Europea Miguel de Cervantes, Valladolid, Spain, (3)University of the Basque Country, Fisica Aplicada I, Donostia, Spain, (4)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (5)University of California Berkeley, Berkeley, CA, United States, (6)University of Oxford, Oxford, United Kingdom
 
Saturn's Stratospheric Water Vapor Distribution (74730)
Brigette E Hesman, University of Maryland College Park, College Park, MD, United States
 
An Enduring Rapidly Moving Storm as a Guide to Saturn’s Equatorial Jet Complex Structure (62160)
Agustin Sanchez-Lavega1, Michael H Wong2, Amy A Simon3, Ricardo Hueso4, Santiago Perez-Hoyos1, Arrate Antuñano5, Jose Felix Rojas5, Teresa del Rio-Gaztelurrutia5, Naiara Barrado-Izagirre1, Itziar Garate-Lopez4, Enrique Garcia-Melendo6, Jose Francisco Sanz-Requena7, Josep M. Gomez-Forrelad8 and Imke De Pater9, (1)University of the Basque Country, Donostia, Spain, (2)U. Berkeley, Berkeley, United States, (3)NASA, Greenbelt, United States, (4)University of the Basque Country, Fisica Aplicada I, Donostia, Spain, (5)UPV/EHU, Bilbao, Spain, (6)Esteve Duran Observatory Foundation, Seva, Spain, (7)UEM Cervantes, Valladolid, Spain, (8)Obs. Fundacionn E. Duran, Mollet, Spain, (9)University of California Berkeley, Berkeley, CA, United States
 
Jupiter's Zonal Jets and Turbulent Eddies: the Importance of Moist Convective Processes on a Global Scale (69429)
Roland Michael Brendon Young, University of Oxford, Atmospheric, Oceanic and Planetary Physics, Department of Physics, Oxford, United Kingdom and Peter L Read, University of Oxford, Oxford, 0X1, United Kingdom
 
Method for Calculating Uncertainty in Automated Cloud-tracking Wind Measurements (72642)
John Blalock, Hampton University, Hampton, VA, United States
 
Numerical Simulations of 1990 Saturn’s Giant Storm (64775)
Enrique Garcia-Melendo, University of the Basque Country, Applied Physics I, Bilbao, Spain; Esteve Duran Observatory Foundation, Seva, Spain and Agustin Sanchez-Lavega, University of the Basque Country (UPV/EHU), Bilbao, Spain
 
Deep Plume Interaction with Gas Giant Weather Layers: Applications to Jupiter and Saturn (72217)
Morgan E O'Neill, Yohai Kaspi and Eli Galanti, Weizmann Institute of Science, Rehovot, Israel
 
Belt-Zone Contrasts in Vertical Motion and Cloud Structure in Jupiter's Troposphere (83521)
Tapio Schneider, ETH Swiss Federal Institute of Technology Zurich, Zurich, Switzerland
 
Zonal Flow and Vortices in Anelastic Deep Convection Models of Jupiter and Saturn With Shallow Stable Stratification (81334)
Moritz H Heimpel1, Johannes Wicht2 and Thomas Gastine2, (1)University of Alberta, Physics Department, Edmonton, AB, Canada, (2)Max Planck Institute for Solar System Research, Göttingen, Germany
 
JunoCam: Science and Outreach Opportunities with Juno (73896)
Candice J Hansen, Planetary Science Institute Tucson, Tucson, AZ, United States
 
Properties of Discrete and Axisymmetric Features in Jupiter’s Atmosphere from Observations of Thermal Emission: Recent Updates on the Eve of the Juno Mission Arrival at Jupiter (65039)
Glenn S Orton1, Leigh N. Fletcher2, Rohini Giles3, James Sinclair1, Thomas K Greathouse4, Thomas Momary5, Padma A Yanamandra-Fisher6, Takuya Fujiyoshi7, Brendan Fisher1, Anna Payne8, Raiyan Seede9, Jason Simon10, Matthew Lai11, Marian Nguyen12, Joshua Fernandez12 and Kevin H Baines13, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (3)University of Oxford, Oxford, United Kingdom, (4)Southwest Research Institute, San Antonio, TX, United States, (5)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (6)Space Science Institute Rancho Cucamonga, Rancho Cucamonga, CA, United States, (7)Subaru Telescope, Hilo, HI, United States, (8)Wellesley College, Wellesley, MA, United States, (9)University of Paris, Abu Dhabi, Abu Dhabi, United Arab Emirates, (10)California Institute of Technology, Pasadena, CA, United States, (11)California State University Pomona, Pomona, CA, United States, (12)California State University Long Beach, Long Beach, CA, United States, (13)Jet Propulsion Laboratory, Pasadena, CA, United States
 
A Long-lived and Color Changing Oval on Jupiter’s NTrZ (at 19ºN) (61825)
Naiara Barrado-Izagirre1, Jon Legarreta1, Agustin Sanchez-Lavega1, Ricardo Hueso2, Santiago Perez-Hoyos1, Jose F Rojas1 and Inigo Mendikoa1,3, (1)University of the Basque Country, Donostia, Spain, (2)University of the Basque Country, Fisica Aplicada I, Donostia, Spain, (3)Tecnalia, Bilbao, Spain
 
The possibility of inferring the depth of Jupiter's Great Red Spot with the Juno gravity experiment (81750)
Marzia Parisi1, Luciano Iess2, Stefano Finocchiaro3, Yohai Kaspi1 and Eli Galanti1, (1)Weizmann Institute of Science, Rehovot, Israel, (2)Univ. La Sapienza, Roma, Italy, (3)Sapienza University of Rome, Rome, Italy
 
Global Response of the Upper Thermosphere to Large Ion Drifts in the Jovian Ovals (64433)
Tariq Majeed1,2, Stephen W Bougher2, Aaron J Ridley3, Randy Gladstone4, Jack H Waite Jr5 and Jared Micheal Bell6, (1)American University of Sharjah, Physics, Sharjah, United Arab Emirates, (2)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (3)University of Michigan Ann Arbor, AOSS, Ann Arbor, MI, United States, (4)Southwest Research Inst, San Antonio, TX, United States, (5)Southwest Research Institute San Antonio, San Antonio, TX, United States, (6)National Institute of Aerospace, Yorktown, VA, United States
 
DEEP ATMOSPHERES OF SATURN AND JUPITER OBSERVED FROM ORBITING SPACECRAFT (75434)
Michael A Janssen, NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
Limits on the Core Mass of Jupiter (75910)
David J Stevenson, California Institute of Technology, Pasadena, CA, United States
 
Long-term Observations of Jovian Mid-Infrared Aurora, Hydrocarbon Abundances, and Temperature: Ground-based and Space-based Comparison and Preparation for Juno (80429)
Theodor Kostiuk1, Tilak Hewagama1,2, Timothy A Livengood1,3, Kelly Elizabeth Fast4, Gordon L Bjoraker5, Ronald C. Carlson6 and Frank Schmuelling7, (1)NASA Goddard SFC, Greenbelt, MD, United States, (2)University of Maryland College Park, Greenbelt, MD, United States, (3)University of Maryland College Park, College Park, MD, United States, (4)NASA Headquarters, Washington, DC, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)Catholic University of America, Washington, DC, United States, (7)German Aerospace Center DLR Bonn, Bonn, Germany
 
Multi-parameter Correlation of Jovian Radio Emissions with Solar Wind and Interplanetary Magnetic Field Data (86176)
Robert J. MacDowall, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Forecasting Juno Microwave Radiometer Observations of Jupiter's Synchrotron Emission from Data Reconstruction Methods and Theoretical Model (68327)
Daniel Santos-Costa1, Scott J Bolton2, Virgil Adumitroaie3, Mike Janssen3, Steve Levin3, Robert J. Sault4, Imke De Pater5 and Chihiro Tao6, (1)Southwest Research Institute San Antonio, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)Jet Propulsion Laboratory, Pasadena, CA, United States, (4)University of Melbourne, Parkville, Australia, (5)University of California Berkeley, Berkeley, CA, United States, (6)IRAP, Toulouse, France
 
Jupiter - Solid or Gaseous? Ask Juno (63425)
John A Ackerman Jr, Angiras Institute, Ottsville, PA, United States
 
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