P33F:
Results from the Investigation of Jupiter’s Atmosphere by Juno and a Supporting Campaign of Earth-Based Observations II Posters


Submit an Abstract to this Session


Session ID#: 51278

Session Description:
NASA’s Juno mission operates a spacecraft in 53-day polar orbits around Jupiter, with the ultimate goals of understanding Jupiter’s origin and evolution.  One specific objective is to establish the structure, composition and dynamics of the deep atmosphere and its relationship with the upper atmosphere.   Juno’s polar orbit with close approaches near the terminator only a few thousand kilometers above the cloud tops provides the opportunity to characterize poorly explored polar regions and to study the characteristics of cloud dynamics and composition at spatial resolutions as fine as 6 km.   An integral part of Juno’s exploration is a campaign of Earth-based observations that extend and enhance spacecraft results by complementing Juno’s spatial, temporal and spectral coverage.  This session welcomes presentations involving all results obtained by and in support of the Juno mission, including not only results of Juno and Earth-supporting observations but also theoretical modeling of atmospheric structure, composition and dynamics.
Primary Convener:  Glenn S Orton, Jet Propulsion Laboratory, Pasadena, CA, United States
Conveners:  Scott J Bolton, Southwest Research Institute, San Antonio, United States, Cheng Li, California Institute of Technology, Pasadena, CA, United States and Gordon L Bjoraker, NASA, Greenbelt, United States
Primary Liaison:  Glenn S Orton, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Chairs:  Cheng Li, California Institute of Technology, Pasadena, CA, United States and Gordon L Bjoraker, NASA, Greenbelt, United States
OSPA Liaison:  Gordon L Bjoraker, NASA, Greenbelt, United States

Cross-Listed:
  • A - Atmospheric Sciences
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]

Abstracts Submitted to this Session:

Juno's Surprising Results and the Impact to Future Exploration (387049)
Scott J Bolton, Southwest Research Institute, San Antonio, United States, Alberto Adriani, INAF-IAPS, Rome, Italy, John E P Connerney, Space Research Corporation, Annapolis, United States, Candice J. Hansen, Planetary Science Institute, Tucson, United States, Andrew P. Ingersoll, California Institute of Technology, Pasadena, CA, United States, Michael A Janssen, Jet Propulsion Laboratory, Pasadena, CA, United States, Steven Levin, Jet Propulsion Laboratory, Pasadena, United States, Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, David J Stevenson, California Institute of Technology, Pasadena, United States and The Juno Science Team
Jupiter’s High-Altitude Hazes as Observed by JunoCam (394040)
Glenn S Orton, Jet Propulsion Laboratory, Pasadena, CA, United States, John Rogers, British Astronomical Association, London, United Kingdom, G. Eichstädt, Independent scholar, Stuttgart, Germany, Candice J. Hansen, Planetary Science Institute, Tucson, United States, Thomas Momary, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and Fachreddin Tabataba-Vakili, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, Spain
Microwave observations of Jupiter’s atmosphere from 1 bar to 200 bars (400073)
Cheng Li1, Fabiano A Oyafuso2, Shannon Thomas Brown3, Virgil Adumitroaie3, Amadeo Bellotti4, John K. Arballo5, Yury Salavatovich Aglyamov1, Michael Allison6, Sushil K Atreya7, Samuel Gulkis5, Andrew P. Ingersoll1, Michael A Janssen5, Jonathan I Lunine8, Sidharth Misra9, Glenn S Orton2, Daniel Santos-Costa10, Edwin Sarkissian5, Paul G Steffes11, Steven Levin12 and Scott J Bolton13, (1)California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (4)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (5)Jet Propulsion Laboratory, Pasadena, CA, United States, (6)NASA Goddard Institute for Space Studies, New York, United States, (7)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, United States, (8)Cornell University, Department of Astronomy, Ithaca, NY, United States, (9)NASA Jet Propulsion Laboratory, Pasadena, United States, (10)Southwest Research Institute San Antonio, San Antonio, TX, United States, (11)Georgia Inst Technology, Atlanta, GA, United States, (12)Jet Propulsion Laboratory, Pasadena, United States, (13)Southwest Research Institute, San Antonio, United States
Ammonia, water vapor, and clouds in Jupiter's Equatorial Zone (419043)
Gordon L Bjoraker, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Michael H. Wong, University of California, Berkeley, United States, Imke De Pater, University of California Berkeley, Departments of Astronomy and of Earth and Planetary Science, Berkeley, United States, Mate Adamkovics, Clemson University, Department of Physics and Astronomy, Clemson, United States, Tilak Hewagama, University of Maryland College Park, College Park, MD, United States and Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States
Juno and the New Renaissance (382218)
Theodore Clarke, JUNO Mission, Altadena, CA, United States
Polygonal patterns of cyclonic vortices at Jupiter poles: Results of a shallow water model (420146)
Harriet K Brettle, Cheng Li and Andrew P. Ingersoll, California Institute of Technology, Pasadena, CA, United States
Non-Hydrostatic Modeling Jupiter’s Cloud Formation and Tropospheric Dynamics in the Juno Era (376040)
Huazhi Ge, University of California Santa Cruz, Earth and Planetary Sciences, Santa Cruz, United States, Cheng Li, California Institute of Technology, Pasadena, CA, United States, Xi Zhang, University of California Santa Cruz, Earth and Planetary Sciences, Santa Cruz, CA, United States and Dongwook Lee, University of California Santa Cruz, Applied Mathematics & Statistics, Santa Cruz, CA, United States
Observations of Jupiter lightning-induced electromagnetic waves from the Juno Waves investigation (383892)
Masafumi Imai1, Ivana Kolmasova2,3, Shannon Thomas Brown4, Ondrej Santolik2,5, William S Kurth6, Michael A Janssen7, George B Hospodarsky6, Donald A Gurnett1, Scott J Bolton8, John E P Connerney9 and Steven Levin10, (1)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (2)Department of Space Physics, Institute of Atmospheric Physics of the Czech Academy of Sciences, Prague, Czech Republic, (3)Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)Charles University, Faculty of Mathematics and Physics, Prague, Czech Republic, (6)University of Iowa, Iowa City, IA, United States, (7)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (8)Southwest Research Institute, San Antonio, United States, (9)Space Research Corporation, Annapolis, United States, (10)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Cyclone-related lightning near Juno's 6th orbit (403962)
Michael H. Wong, University of California Berkeley, Berkeley, CA, United States, Shannon Thomas Brown, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Leigh N. Fletcher, University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, Gordon L Bjoraker, NASA, Greenbelt, United States, Imke De Pater, University of California Berkeley, Departments of Astronomy and of Earth and Planetary Science, Berkeley, United States and Amy A Simon, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Mid-infrared spectra and images of Jupiter’s auroral regions during perijoves 11 – 15 (466713)
James Andrew Sinclair1, Glenn Orton2, Thomas K Greathouse3, Rohini Giles4, Yasumasa Kasaba5, Takao M Sato6, Haruna Watanabe7, Chihiro Tao8, Randy Gladstone3, George B Clark9, Leigh N. Fletcher10, Julianne I Moses11, Patrick GJ Irwin12 and Fachreddin Tabataba-Vakili13, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (3)Southwest Research Institute, San Antonio, United States, (4)University of Oxford, Oxford, United Kingdom, (5)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (6)ISAS, Tokyo, Japan, (7)Tohoku University, Sendai, Japan, (8)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (9)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (10)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (11)Space Science Institute, Boulder, United States, (12)University of Oxford, Atmospheric, Oceanic, and Planetary Physics laboratory, Oxford, United Kingdom, (13)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, Spain
High energy radiation profile of Jupiter as observed by the Juno ASC (433764)
Finn Eskemann Jørgensen1, John Leif Joergensen2, Peter S Joergensen3, Matija Herceg4, Troelz Denver4, Mathias Benn2, Julia Sushkova4, John E P Connerney5, Ronald J Oliversen6, Daniel J Gershman7, Stavros Kotsiaros4, Scott J Bolton8 and Steven Levin9, (1)DTU National Space Institute, København Ø, Denmark, (2)Technical University of Denmark, DTU Space, Lyngby, Denmark, (3)DTU Space, National Space Institute, Technical University of Denmark, Kgs Lyngby, Denmark, (4)Technical University of Denmark, DTU Space, Kgs. Lyngby, Denmark, (5)Space Research Corporation, Annapolis, United States, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)NASA Goddard Space Flight Center, Greenbelt, United States, (8)Southwest Research Institute, San Antonio, United States, (9)Jet Propulsion Laboratory, Pasadena, United States
Cloud Morphology Associated with Jovian Lightning (452009)
Shannon Thomas Brown, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Michael A Janssen, Jet Propulsion Laboratory, Pasadena, CA, United States, Sushil K Atreya, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, United States, Scott J Bolton, Southwest Research Institute, San Antonio, United States, Andrew P. Ingersoll, California Institute of Technology, Pasadena, CA, United States, Steven Levin, Jet Propulsion Laboratory, Pasadena, United States, Cheng Li, Caltech, Pasadena, United States, Jonathan I Lunine, Cornell University, Department of Astronomy, Ithaca, NY, United States, Glenn S Orton, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States and Paul G Steffes, Georgia Institute of Technology Main Campus, Atlanta, GA, United States
Towards improved simulations of the Jovian synchrotron radiation belts as seen by Juno’s MWR (455876)
Virgil Adumitroaie1, John K. Arballo2, Shannon Thomas Brown1, Sam Gulkis2, Steven Levin3, Michael A Janssen2, Glenn Orton4, Fabiano A Oyafuso3, Cheng Li5, Andrew P. Ingersoll5, Michael D Allison6, John E P Connerney7, Paul G Steffes8, Sushil K Atreya9, Scott J Bolton10 and Daniel Santos-Costa11, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Jet Propulsion Laboratory, Pasadena, United States, (4)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (5)California Institute of Technology, Pasadena, CA, United States, (6)Goddard Institute of Space Studies, New York, NY, United States, (7)Space Research Corporation, Annapolis, United States, (8)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (9)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, United States, (10)Southwest Research Institute, San Antonio, United States, (11)Southwest Research Institute, San Antonio, TX, United States
How Deep is the Great Red Spot? Determining the Depth of the GRS with the Juno Gravity Measurements (406083)
Eli Galanti1, Marzia Parisi2, Yohai Kaspi1 and William M Folkner3, (1)Weizmann Institute of Science, Earth and Planetary Sciences, Rehovot, Israel, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
Contemporaneous VLA and ALMA observations of Jupiter during the Juno mission (371449)
Imke De Pater, University of California Berkeley, Departments of Astronomy and of Earth and Planetary Science, Berkeley, United States, Robert J. Sault, University of Melbourne, Parkville, Australia, Chris Moeckel, Space Sciences Laboratory, Berkeley, United States, Arielle Moullet, SOFIA/USRA, Moffett Field, CA, United States, Bryan J Butler, National Radio Astronomy Observatory, Socorro, NM, United States, Leigh N. Fletcher, University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, David deBoer, University of California, Berkeley, CA, United States, Michael H. Wong, University of California, Berkeley, United States, Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, Michael A Janssen, Jet Propulsion Laboratory, Pasadena, CA, United States, Eric Villard, ALMA, Santiago, Chile and Gordon L Bjoraker, NASA, Greenbelt, United States
High-Resolution Near-Infrared Mapping of Jupiter's Clouds in Support of the Juno Mission (410851)
Rohini Giles1, Glenn Orton2, Andrew Stephens3, Thomas Momary4 and James Andrew Sinclair2, (1)Southwest Research Institute, San Antonio, United States, (2)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (3)Gemini Observatory, Hilo, United States, (4)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
Radiative Transfer Analysis of Hyperspectral Image Cubes of Jupiter Acquired During Juno’s 13th Perijove Pass (400586)
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, Oakland, CA, United States, Robert Hull, New Mexico State University Main Campus, Department of Electrical and Computer Engineering, Las Cruces, United States, Paul Strycker, University of Wisconsin Platteville, Platteville, WI, United States and Kevin H Baines, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
NASA/IRTF Near-Infrared Spectroscopy and Imaging of Jupiter in Support of the Juno Mission (429245)
Kevin H Baines, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, Thomas Momary, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, Rohini Giles, Jet Propulsion Laboratory/ California Institute of Technology, Pasadena, United States, Laura D Hu, California Institute of Technology, Pasadena, CA, United States, Vishnu Santhosh, University of Texas at Austin, Austin, TX, United States and Sandra C Wells, Universitat Politècnica de Catalunya, Barcelona, Spain
Observations of Jupiter’s low-latitude ionosphere: almost-global maps of H3+ temperature and density (444255)
James O'Donoghue, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Luke Moore, Boston University, Astronomy; Center for Space Physics, Boston, United States, Tom Stallard, Northumbria University, Newcastle-Upon-Tyne, United Kingdom and John E P Connerney, Space Research Corporation, Annapolis, United States
Application of GIS-related and Statistical Techniques to Jovian Atmosphere (460869)
Padma A Yanamandra-Fisher, Space Science Institute Rancho Cucamonga, Rancho Cucamonga, CA, United States, Eric Sussenbach, ESRI, Willemstad, Barbados, Andrew Casely, The PACA Project, Sydney, Australia and Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States

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