P33C:
Juno's Exploration of Jupiter and the Earth-Based Collaborative Campaign III Posters

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Session ID#: 13297

Session Description:
NASA's Juno mission to Jupiter launched in 2011 and arrived at Jupiter on July 4, 2016. Juno's scientific objectives include the study of Jupiter's interior, atmosphere and magnetosphere with the goal of understanding Jupiter's origin, formation and evolution.  An extensive campaign of Earth based observations of Jupiter and the solar wind were orchestrated to complement Juno measurements during Juno's approach to Jupiter and during its orbital mission around Jupiter.  This session provides results from the Juno measurements and the collaborative campaign during the early phases of Juno's prime mission.  Scientific results include Jupiter's interior structure, magnetic field, deep atmospheric dynamics and composition, and the first in-situ exploration of Jupiter's polar magnetosphere and aurorae.
Primary Convener:  Scott J Bolton, Southwest Research Institute, San Antonio, United States
Conveners:  John E P Connerney, NASA Goddard Space Flight Center, Greenbelt, United States, Glenn S Orton, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States and Fran Bagenal, University of Colorado at Boulder, Boulder, CO, United States
Chairs:  John E P Connerney, NASA Goddard Space Flight Center, Greenbelt, United States and Scott J Bolton, Southwest Research Institute, San Antonio, United States
OSPA Liaison:  Glenn S Orton, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Co-Organized with:
SPA-Magnetospheric Physics, and SPA-Magnetospheric Physics

Cross-Listed:
  • SH - SPA-Solar and Heliospheric Physics
  • SM - SPA-Magnetospheric Physics

Proposed Co-Organized Session with:
  • SM - SPA-Magnetospheric Physics
Index Terms:

2704 Auroral phenomena [MAGNETOSPHERIC PHYSICS]
2756 Planetary magnetospheres [MAGNETOSPHERIC PHYSICS]
5724 Interiors [PLANETARY SCIENCES: FLUID PLANETS]
6220 Jupiter [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Abstracts Submitted to this Session:

Juno, The Cultural Connection (188598)
Theodore Clarke, JUNO Mission, Altadena, CA, United States
Continuous Monitoring of Jupiter's Aurora and Io Plasma Torus with the Hisaki Satellite during Joint Observing Campaign with Juno (145565)
Tomoki Kimura1, Atsushi Yamazaki2, Go Murakami3, George B Clark4, Fuminori Tsuchiya5, Kazuo Yoshioka6, Chihiro Tao7, Hajime Kita5, Masaki Fujimoto2, Jonathan D Nichols8, Sarah Victoria Badman9 and Denis C Grodent10, (1)RIKEN, Wako, Japan, (2)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (3)Japan Aerospace Exploration Agency, Kanagawa, Japan, (4)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (5)Tohoku University, Sendai, Japan, (6)University of Tokyo, Bunkyo-ku, Japan, (7)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (8)University of Leicester, School of Physics and Astronomy, Leicester, LE1, United Kingdom, (9)University of Lancaster, Lancaster, United Kingdom, (10)Université de Liège, LPAP - STAR Institute, Liege, Belgium
The complex behavior of the satellite footprints at Jupiter: the result of universal processes? (146988)
Bertrand Bonfond1, Denis C Grodent1, Sarah Victoria Badman2, Joachim Saur3, Dmitry Bisikalo4, Valery Shematovich4, Jean-Claude M. C. Gerard5, Katerina Radioti1, Randy Gladstone6, Maarten H Versteeg6, Thomas Greathouse6, Vincent Hue7, Michael Wayne Davis7, Scott J Bolton6, Steven Levin8, John E P Connerney9 and Fran Bagenal10, (1)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (2)University of Lancaster, Lancaster, United Kingdom, (3)University of Cologne, Institute of Geophysics and Meteorology, Cologne, Germany, (4)Institute of Astronomy, Moskow, Russia, (5)Université de Liège, Liege, Belgium, (6)Southwest Research Institute, San Antonio, United States, (7)Southwest Research Institute, San Antonio, TX, United States, (8)Jet Propulsion Laboratory, Pasadena, CA, United States, (9)Space Research Corporation, Annapolis, United States, (10)University of Colorado at Boulder, Boulder, CO, United States
The magnetic field in Jupiter's plasma sheet and magnetopause boundary layers (147321)
Daniel J Gershman1, John E P Connerney2, Gina A DiBraccio3, William S Kurth4, George B Hospodarsky4, Barry Mauk5 and Philip W Valek6, (1)University of Maryland College Park, College Park, United States, (2)Space Research Corporation, Annapolis, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)University of Iowa, Iowa City, IA, United States, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (6)Southwest Research Institute, San Antonio, TX, United States
Statistical study of solar wind control on Jovian UV auroral activity obtained from long-term Hisaki EXCEED observations (153639)
Hajime Kita1, Tomoki Kimura2, Chihiro Tao3, Fuminori Tsuchiya1, Atsushi Yamazaki4, Go Murakami5, Kazuo Yoshioka6, Hiroaki Misawa1, Takeshi Sakanoi7, Yasumasa Kasaba8, Ichiro Yoshikawa9 and Masaki Fujimoto4, (1)Tohoku University, Sendai, Japan, (2)RIKEN, Wako, Japan, (3)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (4)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (5)Japan Aerospace Exploration Agency, Kanagawa, Japan, (6)University of Tokyo, Bunkyo-ku, Japan, (7)PPARC, Tohoku University, Sendai, Japan, (8)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (9)The University of Tokyo, Tokyo, Japan
First Hubble Space Telescope Movies of Jupiter’s Ultraviolet Aurora During the NASA Juno Prime Mission (130387)
Denis C Grodent1, Randy Gladstone2, John T Clarke3, Bertrand Bonfond1, Jean-Claude M. C. Gerard4, Katerina Radioti1, Jonathan D Nichols5, Emma J Bunce6, Lorenz Roth7, Joachim Saur8, Tomoki Kimura9, Glenn S Orton10, Sarah Victoria Badman11, Barry Mauk12, John E P Connerney13, William S Kurth14, Alberto Adriani15, Candice J Hansen16, Scott J Bolton2, Steven Levin17 and Fran Bagenal18, (1)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (2)Southwest Research Institute, San Antonio, United States, (3)Boston University, Boston, MA, United States, (4)Université de Liège, Liege, Belgium, (5)University of Leicester, School of Physics and Astronomy, Leicester, LE1, United Kingdom, (6)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (7)KTH Royal Institute of Technology, Stockholm, Sweden, (8)University of Cologne, Institute of Geophysics and Meteorology, Cologne, Germany, (9)RIKEN, Wako, Japan, (10)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (11)University of Lancaster, Lancaster, United Kingdom, (12)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (13)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (14)University of Iowa, Iowa City, IA, United States, (15)INAF-IAPS, Rome, Italy, (16)Planetary Science Institute Tucson, Tucson, AZ, United States, (17)Jet Propulsion Laboratory, Pasadena, United States, (18)University of Colorado at Boulder, Boulder, CO, United States
Observations of Jupiter's Low-Frequency Radio Emissions from the Juno Waves Instrument in Collaboration with the Earth-Based Radio Telescopes (148738)
Masafumi Imai1, William S Kurth2, George B Hospodarsky2, Scott J Bolton3, John E P Connerney4, Steven Levin5, Philippe M Zarka6, Baptiste Cecconi7, Alain Lecacheux8 and Laurent Lamy7, (1)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (2)University of Iowa, Iowa City, IA, United States, (3)Southwest Research Institute, San Antonio, United States, (4)Space Research Corporation, Annapolis, United States, (5)Jet Propulsion Laboratory, Pasadena, CA, United States, (6)Observatoire de Paris, PSL, CNRS, LESIA, Meudon, France, (7)Paris Observatory Meudon, Meudon, France, (8)Paris Observatory Meudon, LIRA, Meudon, France
The strength and evolution of stratospheric-auroral processes on Jupiter, as observed by IRTF-TEXES (168592)
James Andrew Sinclair1, Glenn S Orton2, Thomas K Greathouse3, Leigh N. Fletcher4, Julianne I Moses5, Vincent Hue3, Patrick GJ Irwin6, Henrik Melin7 and Rohini Giles8, (1)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)Southwest Research Institute, San Antonio, TX, United States, (4)University of Leicester, Leicester, United Kingdom, (5)Space Science Institute Seabrook, Seabrook, TX, United States, (6)University of Oxford, Atmospheric, Oceanic, and Planetary Physics laboratory, Oxford, United Kingdom, (7)University of Leicester, Leicester, LE1, United Kingdom, (8)University of Oxford, Oxford, United Kingdom
Feasibility of Juno radio occultations of the Io plasma torus (178300)
Phillip H Phipps, Boston University, Boston, MA, United States and Paul Withers, Boston University, Boston, United States
Jupiter’s Auroral Energy Input Observed by Hisaki/EXCEED and its Modulations by Io’s Volcanic Activity (179669)
Chihiro Tao1, Tomoki Kimura2, Fuminori Tsuchiya3, Go Murakami4, Kazuo Yoshioka5, Hajime Kita3, Atsushi Yamazaki6, Yasumasa Kasaba7, Ichiro Yoshikawa8 and Masaki Fujimoto6, (1)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (2)RIKEN, Wako, Japan, (3)Tohoku University, Sendai, Japan, (4)Japan Aerospace Exploration Agency, Kanagawa, Japan, (5)University of Tokyo, Bunkyo-ku, Japan, (6)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (7)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (8)The University of Tokyo, Tokyo, Japan
Properties of Jupiter’s auroral acceleration region inferred with HST-STIS spectral images (183271)
Licia C Ray, Mullard Space Science Laboratory, Dorking, United Kingdom, Christopher Stephen Arridge, University College London, Mullard Space Science Laboratory, London, United Kingdom, Jacques Gustin, Université de Liège, Liège, Belgium and Denis C Grodent, Université de Liège, LPAP - STAR Institute, Liege, Belgium
Modeling the Jovian Magnetopause in Support of Juno (148769)
Adam Masters, Imperial College London, Blackett Laboratory, London, United Kingdom
X-ray Monitoring of the Jovian Polar Aurora during Juno Approach (184281)
Ralph Kraft, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, Caitriona Mary Jackman, University of Southampton, Southampton, United Kingdom, William Dunn, University College London, Department of Phyics and Astronomy, London, United Kingdom, Graziella Branduardi-Raymont, University College London, Mullard Space Science Laboratory, London, United Kingdom, Randy Gladstone, Southwest Research Institute, San Antonio, United States, Tomoki Kimura, RIKEN, Wako, Japan, Ronald Elsner, NASA Marshall Space Flight Center, Huntsville, AL, United States, Jonathan D Nichols, University of Leicester, School of Physics and Astronomy, Leicester, LE1, United Kingdom and Licia C Ray, Mullard Space Science Laboratory, Dorking, United Kingdom
Variability of Mid-Infrared Aurora on Jupiter: 1979 to 2016 (194772)
Theodor Kostiuk1, Timothy A Livengood2, Tilak Hewagama3, Kelly Elizabeth Fast4, Gordon L Bjoraker5, Frank Schmuelling6, Guido Sonnabend7 and John R. Kolasinski1, (1)NASA Goddard SFC, Greenbelt, MD, United States, (2)University of Maryland College Park, Astronomy, College Park, MD, United States, (3)University of Maryland, College Park, Astronomy, College Park, MD, United States, (4)NASA Headquarters, Washington, DC, United States, (5)NASA Goddard Space Flight Center, Greenbelt, United States, (6)German Aerospace Center DLR Bonn, Bonn, Germany, (7)U. Cologne/RPG, Meckenheim, Germany
Scales of wave-particle interaction processes in Jupiter's magnetosphere: Implications for JUNO/JEDI measurements (126574)
Joachim Saur, University of Cologne, Cologne, Germany, Anne Schreiner, University of Cologne, Institute of Geophysics and Meteorology, Cologne, Germany and Barry Mauk, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Jupiter’s distant magnetic equator region in energetic charged particle data (133736)
Chris Paranicas1, Barry Mauk1, Dennis K Haggerty2, George B Clark3, Peter Kollmann1, Abigail M Rymer4, John E P Connerney5, Fran Bagenal6, Scott J Bolton7 and Steven Levin8, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Johns Hopkins Univ, Laurel, MD, United States, (3)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (5)Space Research Corporation, Annapolis, United States, (6)University of Colorado at Boulder, Boulder, CO, United States, (7)Southwest Research Institute, San Antonio, United States, (8)Jet Propulsion Laboratory, Pasadena, United States
Accelerated Flows at Jupiter’s Magnetopause: Evidence for Magnetic Reconnection Along the Dawn Flank (136219)
Robert W Ebert1, Frederic Allegrini2,3, Scott J Bolton3, Fran Bagenal4, John E P Connerney5, George B Clark6, William S Kurth7, Steven Levin8, Philippe Louarn9, Barry Mauk10, David J McComas1,11, Michelle L Reno1,12, Michelle F Thomsen13, Philip W Valek1,14, Scott Weidner15 and Robert J Wilson16, (1)Southwest Research Institute, San Antonio, TX, United States, (2)University of Texas at San Antonio, Department of Physics & Astronomy, San Antonio, TX, United States, (3)Southwest Research Institute, San Antonio, United States, (4)University of Colorado at Boulder, Boulder, CO, United States, (5)Space Research Corporation, Annapolis, United States, (6)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (7)University of Iowa, Iowa City, IA, United States, (8)Jet Propulsion Laboratory, Pasadena, United States, (9)IRAP, Toulouse, France, (10)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (11)Princeton University, Department of Astrophysical Sciences and Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (12)Austin Mission Consulting, Austin, TX, United States, (13)Planetary Science Institute Tucson, Tucson, AZ, United States, (14)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, TX, United States, (15)Princeton University, Princeton, NJ, United States, (16)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
Interaction of Jovian energetic particles with moons and gas tori based on recent Juno/JEDI data (148694)
Peter Kollmann1, Barry Mauk1, George B Clark2, Chris Paranicas1, Dennis K Haggerty3, Abigail M Rymer4, Scott J Bolton5, John E P Connerney6 and Steven Levin7, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (3)Johns Hopkins Univ, Laurel, MD, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (5)Southwest Research Institute, San Antonio, United States, (6)Space Research Corporation, Annapolis, United States, (7)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
The Juno Jupiter Energetic Particle Detector Instrument (JEDI) Investigation Data Structures and Analysis Tools (151574)
Lawrence E Brown1, James M Peachey1, Jon Duane Vandegriff1, Barry Mauk1, Dennis K Haggerty2, Chris Paranicas1, George B Clark3, Peter Kollmann1 and Abigail M Rymer4, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Johns Hopkins Univ, Laurel, MD, United States, (3)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, United States
First steps toward data assimilation of Jupiter's radiation belts using Juno and radio observations and physics-based models (157673)
Daniel Santos-Costa1, Scott J Bolton2, George B Clark3, Peter Kollmann4, Barry Mauk4, Fran Bagenal5, Heidi N Becker6, Mike Janssen7, Steven Levin6, Fabiano A Oyafuso8, Virgil Adumitroaie9, Julien N Girard10, Philippe M Zarka11, Andrew P. Ingersoll12, William S Kurth13 and John E P Connerney14, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, United States, (3)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)University of Colorado at Boulder, Boulder, CO, United States, (6)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (7)Jet Propulsion Laboratory, Pasadena, CA, United States, (8)Jet Propulsion Laboratory, Pasadena, United States, (9)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (10)CEA/SAp/Irfu, AIM, Saclay, France, (11)Observatoire de Paris, PSL, CNRS, LESIA, Meudon, France, (12)California Institute of Technology, Pasadena, CA, United States, (13)University of Iowa, Iowa City, IA, United States, (14)Space Research Corporation, Annapolis, United States
A 1D Forward Model of Solar Wind Conditions Using JADE-I (160542)
Robert J Wilson1, Fran Bagenal2, Philip W Valek3, David J McComas4, Scott J Bolton5, Frederic Allegrini5, Nigel G Angold6, John E P Connerney7, Kyung Chae3, Robert W Ebert3, Thomas K Kim3,8, Steven Levin9, Chad E Loeffler3, Philippe Louarn10, Drake A Ranquist11, Michelle L Reno3, Jamey Szalay3, Scott Weidner12 and Jenna Lynn Zink8, (1)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (2)University of Colorado at Boulder, Boulder, CO, United States, (3)Southwest Research Institute, San Antonio, TX, United States, (4)Princeton University, Office of the VP for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (5)Southwest Research Institute, San Antonio, United States, (6)Angold Consulting for SwRI, La Cañada, CA, United States, (7)Space Research Corporation, Annapolis, United States, (8)University of Texas at San Antonio, San Antonio, TX, United States, (9)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (10)IRAP, Toulouse, France, (11)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (12)Princeton University, Princeton, NJ, United States
Measurements of the Dawn-side Jovian Magnetosheath by Juno/JADE (169581)
Jamey R Szalay1, Frederic Allegrini2, Fran Bagenal3, Scott J Bolton2, George B Clark4, John E P Connerney5, Robert W Ebert1, William S Kurth6, Steven Levin7, Philippe Louarn8, Barry Mauk9, David J McComas10, Michelle L Reno1, Michelle F Thomsen11, Philip W Valek1, Scott Weidner12 and Robert J Wilson13, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, United States, (3)University of Colorado at Boulder, Boulder, CO, United States, (4)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (5)Space Research Corporation, Annapolis, United States, (6)University of Iowa, Iowa City, IA, United States, (7)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (8)IRAP, Toulouse, France, (9)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (10)Princeton University, Office of the VP for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (11)Planetary Science Institute Tucson, Tucson, AZ, United States, (12)Princeton University, Princeton, NJ, United States, (13)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
Modelling the Auroral Magnetosphere-Ionosphere Coupling System at Jupiter (178688)
Emma J Bunce1, Stanley Cowley2 and G Provan1, (1)University of Leicester, Department of Physics and Astronomy, Leicester, LE1, United Kingdom, (2)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom
JEDI observations of energetic ions in the Jovian polar regions (179769)
Dennis K Haggerty1, Barry Mauk1, Chris Paranicas1, George B Clark2, Peter Kollmann1, Abigail M Rymer3, Scott J Bolton4, John E P Connerney5 and Steven Levin6, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)Southwest Research Institute, San Antonio, United States, (5)Space Research Corporation, Annapolis, United States, (6)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Empirical Modeling of Jovian Electron Distributions Using Juno's MWR Synchrotron Radiation Observations (186172)
Virgil Adumitroaie1, Steven Levin2, Michael A Janssen1, Samuel Gulkis3, Daniel Santos-Costa4 and Scott J Bolton5, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)California Institute of Technology, Pasadena, CA, United States, (4)Southwest Research Institute, San Antonio, TX, United States, (5)Southwest Research Institute, San Antonio, United States
Retrievals of atmospheric parameters from radiances obtained by the Juno Microwave Radiometer (167292)
Cheng Li1, Andrew P. Ingersoll1 and Michael A Janssen2, (1)California Institute of Technology, Pasadena, CA, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States
Calibration and Performance of the Juno Microwave Radiometer during the First Science Orbits (189516)
Shannon Thomas Brown1, Sidharth Misra2, Michael A Janssen1 and Ross Williamson2, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
A Quick-Look Method for the Analysis of Juno Microwave Radiometer Data (191659)
Laura Alisic Jewell, NASA Jet Propulsion Laboratory, Pasadena, United States, Ross Williamson, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, Michael A Janssen, NASA Jet Propulsion Laboratory, Pasadena, CA, United States and Fabiano A Oyafuso, Jet Propulsion Laboratory, Pasadena, United States
Simulation of Antenna Brightness Temperatures for the Juno Microwave Radiometer (191786)
Fabiano A Oyafuso1, Sam Gulkis2, Virgil Adumitroaie3, Michael A Janssen3, Sushil K Atreya4, Shannon Thomas Brown3, Amadeo Bellotti5, Cheng Li6, Andrew P. Ingersoll6, Daniel Santos-Costa7, Ross Williamson8 and Laura Alisic Jewell9, (1)Jet Propulsion Laboratory, Pasadena, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (4)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (5)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (6)California Institute of Technology, Pasadena, CA, United States, (7)Southwest Research Institute, San Antonio, TX, United States, (8)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (9)NASA Jet Propulsion Laboratory, Pasadena, United States
Quicklook Constituent Abundance and Stretch Parameter Retrieval for the Juno Microwave Radiometer using Neural Networks (162413)
Amadeo Bellotti and Paul G Steffes, Georgia Institute of Technology Main Campus, Atlanta, GA, United States
Predicting Juno Evidence for a Solid Methane Gas Hydrate Jupiter J. Ackerman  Abstract (184223)
John A Ackerman Jr, Retired, Washington, DC, United States
Modeling the disequilibrium species for Jupiter and Saturn: Implications for Juno and Saturn entry probe (168126)
Dong Wang, Cornell University, Ithaca, NY, United States, Jonathan I Lunine, California Institute of Technology, Center for Astrophysics and Planetary Science, Pasadena, United States and Olivier Mousis, Aix-Marseille Université, CNRS, CNES, Institut Origines, LAM, Marseille, France
Early Juno Era Optical Imaging and Analysis of Jupiter’s Atmospheric Structure and Color with the NMSU Acousto-optic Imaging Camera (164789)
Emma Dahl, California Institute of Technology, Pasadena, CA, United States, Nancy Chanover, New Mexico State University Main Campus, Department of Astronomy, Las Cruces, NM, United States, David Voelz, New Mexico State University Main Campus, Department of Electrical and Computer Engineering, Las Cruces, NM, United States, David Kuehn, Pittsburg State University, Physics, Pittsburg, KS, United States and Paul Strycker, University of Wisconsin Platteville, Platteville, WI, United States
Transport and mixing of ammonia in Jupiter's atmosphere (187260)
Junjun Liu1, Tapio Schneider2 and Tapio Schneider2, (1)Space Science Institute Boulder, Boulder, CO, United States, (2)ETH Swiss Federal Institute of Technology Zurich, Zurich, Switzerland
A Multi-layered Model for the Shape, Zonal Winds and Gravitational Field of Jupiter (151873)
Gerald Schubert1, Keke Zhang2 and Dali Kong2, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)University of Exeter, Exeter, United Kingdom

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