P021
Jupiter’s Atmosphere through the Eyes of Juno

Session ID#: 83117

Session Description:
NASA's Juno mission operates a spacecraft in 53-day polar orbits around Jupiter, with a goal of understanding Jupiter's origin and evolution.  As the largest and most massive planet in our solar system, Jupiter offers unique insight in the history of our solar system and how planetary systems in general form and evolve.  One objective of the Juno mission is to establish the structure, composition and dynamics of the deep atmosphere and its relationship with the upper atmosphere.  Juno has provided new observations of the global atmospheric structure and composition, storm and lightning distribution and cloud morphology and dynamics.  This session welcomes presentations involving all results obtained by and in support of the Juno mission, including not only results of Juno and Earth-based supporting atmospheric observations but also theoretical modeling of atmospheric structure, composition and dynamics, and comparisons with the atmosphere of Saturn.
Index Terms:

5704 Atmospheres [PLANETARY SCIENCES: FLUID PLANETS]
5739 Meteorology [PLANETARY SCIENCES: FLUID PLANETS]
5754 Polar regions [PLANETARY SCIENCES: FLUID PLANETS]
6220 Jupiter [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Primary Convener:  Shannon Thomas Brown, Jet Propulsion Laboratory, Pasadena, CA, United States
Conveners:  Alessandro Mura, IAPS-INAF, Rome, Italy, Liming Li, Cornell University, Ithaca, NY, United States and F. Tabataba-Vakili, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, Spain
Primary Liaison:  Shannon Thomas Brown, Jet Propulsion Laboratory, Pasadena, CA, United States
 
First Direct Wind Measurements in the Stratosphere of Jupiter (487200)
Thibault Cavalié1,2, Bilal Benmahi1, Raphael Moreno2, Emmanuel Lellouch3, Thierry Fouchet2, Vincent Hue4, Thomas K Greathouse4, Randy Gladstone4, James Andrew Sinclair5, Michel Dobrijevic6, Paul Hartogh7, Christopher Jarchow8 and Ladislav Rezac8, (1)Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, Pessac, France, (2)LESIA, Observatoire de Paris, Meudon, France, (3)LESIA, Observatoire de Paris, Paris, France, (4)Southwest Research Institute, San Antonio, TX, United States, (5)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (6)Laboratoire d'Astrophysique de Bordeaux - Univ. Bordeaux - CNRS, Pessac, France, (7)MPI for Solar System Research, Katlenburg-Lindau, Germany, (8)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany
 
CH4 spatial and vertical distribution in the Jovian atmosphere observed by JIRAM on Juno mission (498502)
Alessandra Migliorini1, Bianca Maria Dinelli2, Francesca Altieri1, Maria Luisa Moriconi2, Alberto Adriani3, Alessandro Mura1, Sushil K Atreya4, Scott J Bolton5, Jean-Claude M C Gerard6, Federico Tosi7, Giuseppe Piccioni1, Roberto Sordini1, Raffaella Noschese1 and Andrea Cicchetti1, (1)IAPS-INAF, Rome, Italy, (2)CNR Institute of Atmospheric Sciences and Climate, Bologna, Italy, (3)Institute for Space Astrophysics and Planetology, Rome, Italy, (4)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (5)Southwest Research Institute, San Antonio, TX, United States, (6)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (7)INAF, Rome, Italy
 
Fine-Scale Waves inJupiter’s Atmosphere Detected by JunoCam (508118)
Glenn S Orton, Jet Propulsion Laboratory, Pasadena, CA, United States, F. Tabataba-Vakili, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, Spain, G. Eichstädt, Independent scholar, Stuttgart, Germany, Candice J. Hansen, Planetary Science Institute, Tucson, AZ, United States, Thomas Momary, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, John Rogers, British Astronomical Association, London, United Kingdom, Andrew P. Ingersoll, California Institute of Technology, Pasadena, CA, United States and Hamish Nicholson, Harvard University, Harvard College, Cambridge, MA, United States
 
A Multi-Spectral Analysis of Recent Perturbations to Jupiter’s Great Red Spot in 2019 (508350)
Thomas Momary1, Glenn S Orton1, James Andrew Sinclair1, Takuya Fujiyoshi2, Mitsuhiko Honda3, John Rogers4, Clyde Foster5, G. Eichstädt6, Arrate Antuñano7, Leigh N. Fletcher7, Nahid Chowdhury7, Tom Stallard8 and Henrik Melin9, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Subaru Telescope, Hilo, HI, United States, (3)Okayama University of Science, Okayama, Japan, (4)British Astronomical Association, London, United Kingdom, (5)Astronomical Society of Southern Africa, Centurion, South Africa, (6)Independent scholar, Stuttgart, Germany, (7)University of Leicester, Leicester, United Kingdom, (8)University of Leicester, Leicester, UNITED KINGDOM, (9)University of Leicester, Leicester, LE1, United Kingdom
 
Numerical Models of the Atmospheric Circulation on Jupiter and Saturn:Zonal Jets, Long-term Variability, and QBO-type Oscillations (511198)
Adam P Showman, University of Arizona, Planetary Sciences, Tucson, AZ, United States, Xianyu Tan, University of Arizona, Tucson, AZ, United States and Xi Zhang, UC Santa Cruz, Earth and Planetary Sciences, Santa Cruz, CA, United States
 
JunoCam Images of Castellanus Clouds on Jupiter (517235)
Candice J Hansen, Planetary Science Institute Tucson, Tucson, AZ, United States, Shawn Brueshaber, Western Michigan University, Kalamazoo, MI, United States, Glenn Orton, Jet Propulsion Laboratory, Pasadena, CA, United States, Thomas Momary, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and Scott J Bolton, Southwest Research Institute, San Antonio, TX, United States
 
Mapping of ultraviolet reflected sunlight from Jupiter using Juno/UVS observations (523013)
Rohini Giles1, Randy Gladstone2, Thomas K Greathouse2, Maarten H Versteeg2, Vincent Hue2, Joshua Kammer2, Michael Wayne Davis2, Scott J Bolton2 and Steven Levin3, (1)Southwest Research Institute, San Antonio, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)Jet Propulsion Laboratory, Pasadena, CA, United States
 
Study of Jovian atmospheric dynamics by a multi-band imaging observation from ground (528995)
Hayate Ito, Meiji university, Kawasaki, Japan, Isshi Tabe, ALPO-JAPAN, Tokyo, Japan, Sumito Hirota, Kawasaki municipal science museum, Kanagawa, Japan and Hidehiko Suzuki, Meiji University, Kawasaki, Japan
 
Initial Results of Juno’s Microwave Imaging of Jupiter’s Atmosphere at Multiple Depths (531490)
Scott J Bolton1, Steven Levin2, Mike Janssen2, Fabiano A Oyafuso3, Zhimeng Zhang4, John K. Arballo2, Cheng Li4, Michael H. Wong5, Glenn Orton2 and The Juno MWR Team, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (4)California Institute of Technology, Pasadena, CA, United States, (5)University of California, Berkeley, CA, United States
 
Jupiter’s Great Red Spot threatened along 2019 by strong interactions with close anticyclones (535753)
Agustin Sanchez-Lavega1, Jon Legarreta1, Ricardo Hueso1, Peio Iñurrigarro1, Jose Felix Rojas1, Santiago Perez-Hoyos1, Jose Francisco Sanz-Requena2 and Inigo Mendikoa3, (1)University of the Basque Country UPV/EHU, Bilbao, Spain, (2)Universidad Europea Miguel de Cervantes, Valladolid, Spain, (3)Tecnalia, Zamudio, Spain
 
JunoCam Cloud Morphology Spatial Structure and Turbulence Spectra (548854)
Justin Garland, Kunio M Sayanagi, John J Blalock, Jacob Gunnarson and Ryan M. McCabe, Hampton University, Hampton, VA, United States
 
Residual Study: Testing Jupiter Atmosphere Models Against Juno MWR Observations (560055)
Zhimeng Zhang1, Virgil Adumitroaie2, Michael D Allison3, John K. Arballo4, Sushil K Atreya5, Heidi N Becker2, Scott J Bolton6, Shannon T. Brown7, John E P Connerney8, Tristan Guillot9, Samuel Gulkis4, Amoree L Hodges10, Andrew P. Ingersoll1, Michael A Janssen4, Steven Levin4, Cheng Li1, Liming Li11, Jonathan I Lunine12, Sidharth Misra13, Glenn Orton4, Fabiano A Oyafuso14, Daniel Santos-Costa15, Edwin Sarkissian4, Paul G Steffes10 and Jack H Waite Jr16, (1)California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (3)Goddard Institute of Space Studies, New York, NY, United States, (4)Jet Propulsion Laboratory, Pasadena, CA, United States, (5)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (6)Southwest Research Institute, San Antonio, TX, United States, (7)NASA Jet Propulsion Laboratory, Pasadena, United States, (8)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (9)Observatoire de la Côte d’Azur, Nice, France, (10)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (11)Cornell University, Ithaca, NY, United States, (12)Cornell University, Department of Astronomy, Ithaca, NY, United States, (13)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (14)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (15)Southwest Research Institute San Antonio, San Antonio, TX, United States, (16)Southwest Research Institute, Space Sciences and Engineering, San Antonio, TX, United States
 
Jupiter As Seen By The Juno Microwave Radiometer: A Progress Report (563724)
Steven Levin1, Virgil Adumitroaie2, Michael D Allison3, John K. Arballo1, Sushil K Atreya4, Heidi N Becker2, Scott J Bolton5, Shannon T. Brown6, John E P Connerney7, Tristan Guillot8, Sam Gulkis9, Amoree L Hodges10, Andrew P. Ingersoll11, Michael A Janssen1, Cheng Li11, Liming Li12, Jonathan I Lunine13, Sidharth Misra14, Glenn S Orton14, Fabiano A Oyafuso15, Daniel Santos-Costa16, Edwin Sarkissian1, Paul G Steffes10, Jack H Waite Jr17 and Zhimeng Zhang11, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (3)Goddard Institute of Space Studies, New York, NY, United States, (4)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (5)Southwest Research Institute, San Antonio, TX, United States, (6)NASA Jet Propulsion Laboratory, Pasadena, United States, (7)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (8)Observatoire de la Côte d’Azur, Nice, France, (9)Shiki, Japan, (10)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (11)California Institute of Technology, Pasadena, CA, United States, (12)University of Houston, Physics Department, Houston, TX, United States, (13)Cornell University, Department of Astronomy, Ithaca, NY, United States, (14)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (15)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (16)Southwest Research Institute San Antonio, San Antonio, TX, United States, (17)Southwest Research Institute, Space Sciences and Engineering, San Antonio, TX, United States
 
Jupiter's Lightning-Associated Clouds: Correlations of Juno Microwave Radiometer Lightning Observations with Cloud Properties Derived from Contemporaneous NASA/IRTFSPeX Camera Images (572235)
Kevin H Baines1, James Andrew Sinclair2, Glenn S Orton2, Thomas Momary3 and Shannon Thomas Brown4, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (4)Jet Propulsion Laboratory, Pasadena, United States
 
Inhibition of moist convection in the atmospheres of Jovian planets: the case of formation of NH4SH by chemical reaction by chemical reaction of NH3 and H2S (580202)
Kensuke Nakajima1, Hiroto Fukunoue1, Ko-ichiro Sugiyama2, Kiyoshi Kuramoto3 and Yoshi-Yuki Hayashi4, (1)Kyushu University, Fukuoka, Japan, (2)National Institute of Technology, Matsue College, Matsue, Japan, (3)Hokkaido University, Sapporo, Japan, (4)Kobe Univ, Kobe, Japan
 
Modeling of Cyclonic Vortices at the Poles of Jupiter (598271)
Cheng Li1, Andrew P. Ingersoll2, Alexandra Klipfel3 and Harriet K Brettle2, (1)University of California Berkeley, Astronomy Department, Berkeley, CA, United States, (2)California Institute of Technology, Pasadena, CA, United States, (3)California Institute of Technology, Geological and Planetary Sciences, Pasadena, United States
 
Measured Elevation of Lightning and Aurora in the Jovian Atmosphere (606495)
Mathias Benn1, John Leif Joergensen1, Troelz Denver1, Matija Herceg1, Peter S Joergensen1, Jose M.G. Merayo1, John E P Connerney2, Scott J Bolton3 and Steven Levin4, (1)DTU Space, National Space Institute, Technical University of Denmark, Kgs Lyngby, Denmark, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)Southwest Research Institute, San Antonio, TX, United States, (4)Jet Propulsion Laboratory, Pasadena, CA, United States
 
Relating Jovian Lightning Rates and Water Abundance: a One-Dimensional Model (613193)
Yury Salavatovich Aglyamov, Cornell University, Ithaca, NY, United States, Jonathan I Lunine, Cornell University, Department of Astronomy, Ithaca, NY, United States, Steven Levin, Jet Propulsion Laboratory, Pasadena, CA, United States, Heidi N Becker, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and Sushil K Atreya, University of Michigan Ann Arbor, Ann Arbor, MI, United States
 
IRTF-TEXES observations of stratospheric CH3 and CH4 emission at Jupiter's high latitudes (617696)
James Andrew Sinclair1, Thomas K Greathouse2, Rohini Giles3, Arrate Antuñano4, Thierry Fouchet5, Bruno Bezard6, George B Clark7, Julianne I Moses8, Vincent Hue2, Glenn S Orton9, Leigh N. Fletcher4 and Patrick GJ Irwin3, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)University of Oxford, Oxford, United Kingdom, (4)University of Leicester, Leicester, United Kingdom, (5)LESIA, Observatoire de Paris, Meudon, France, (6)Paris Observatory Meudon, Meudon, France, (7)Catholic University of America, Washington, DC, United States, (8)Space Science Institute, Seabrook, TX, United States, (9)NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
Characterizing the Variability of Jupiter's Polar Regions (625216)
Angela Burke1, Glenn S Orton2 and James Andrew Sinclair2, (1)University of Alabama in Huntsville, Huntsville, AL, United States, (2)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, CA, United States
 
Calibration Stability of the Juno Microwave Radiometer (625232)
Sidharth Misra1, Shannon Thomas Brown2, Steven Levin3 and Michael A Janssen3, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)Jet Propulsion Laboratory, Pasadena, United States, (3)Jet Propulsion Laboratory, Pasadena, CA, United States
 
A comparative analysis of the deep atmospheric dynamics of Jupiter and Saturn in light of the Juno and Cassini gravity measurements (626511)
Yohai Kaspi1, Eli Galanti1, Adam P Showman2, David J Stevenson3, Tristan Guillot4, Luciano Iess5 and Scott J Bolton6, (1)Weizmann Institute of Science, Rehovot, Israel, (2)University of Arizona, Planetary Sciences, Tucson, AZ, United States, (3)California Institute of Technology, Pasadena, CA, United States, (4)Observatoire de la Côte d’Azur, Nice, France, (5)Univ. La Sapienza, Roma, Italy, (6)Southwest Research Institute, San Antonio, TX, United States
 
Distribution of Storms and Moist Convection on Jupiter derived from Juno MWR data (628205)
Shannon Thomas Brown1, Michael A Janssen1, Sushil K Atreya2, Scott J Bolton3, Andrew P. Ingersoll4, Steven Levin1, Cheng Li4, Jonathan I Lunine5, Glenn Orton1 and Paul G Steffes6, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (3)Southwest Research Institute, San Antonio, TX, United States, (4)California Institute of Technology, Pasadena, CA, United States, (5)Cornell University, Department of Astronomy, Ithaca, NY, United States, (6)Georgia Inst Technology, Atlanta, GA, United States
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