P24B:
Results from the Investigation of Jupiter’s Atmosphere by Juno and a Supporting Campaign of Earth-Based Observations I


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Session ID#: 60221

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:  Scott J Bolton, Southwest Research Institute, San Antonio, United States and Glenn S Orton, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, 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:

Heidi N Becker1, Shannon Thomas Brown2, Masafumi Imai3, Andrew P. Ingersoll4, Martin J Brennan5, James W Alexander5, Alexandre Guillaume1, Candice J. Hansen6, Ivana Kolmasova7,8, William S Kurth9, Michael A Janssen5, Scott J Bolton10, Steven Levin1 and John E P Connerney11, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (4)California Institute of Technology, Pasadena, CA, United States, (5)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (6)Planetary Science Institute, Tucson, United States, (7)Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic, (8)Department of Space Physics, Institute of Atmospheric Physics of the Czech Academy of Sciences, Prague, Czech Republic, (9)University of Iowa, Iowa City, IA, United States, (10)Southwest Research Institute, San Antonio, United States, (11)Space Research Corporation, Annapolis, United States
Steven Levin1, Michael A Janssen1, Scott J Bolton2, John E P Connerney3, Virgil Adumitroaie4, Sushil K Atreya5, Shannon Thomas Brown4, Samuel Gulkis1, Andrew P. Ingersoll6, Cheng Li6, Sidharth Misra7, Glenn S Orton8, Fabiano A Oyafuso8, Daniel Santos-Costa9, Edwin Sarkissian1,8 and Paul G Steffes10, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Southwest Research Institute, San Antonio, United States, (3)Space Research Corporation, Annapolis, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, United States, (6)California Institute of Technology, Pasadena, CA, United States, (7)NASA Jet Propulsion Laboratory, Pasadena, United States, (8)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (9)Southwest Research Institute San Antonio, San Antonio, TX, United States, (10)Georgia Inst Technology, Atlanta, GA, United States
Fachreddin Tabataba-Vakili1, Glenn Orton2, Candice J. Hansen3, John Rogers4, G. Eichstädt5, Thomas Momary6, M. A. Caplinger7, Michael A Ravine7 and Scott J Bolton8, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (3)Planetary Science Institute, Tucson, United States, (4)British Astronomical Association, London, United Kingdom, (5)Independent scholar, Stuttgart, Germany, (6)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (7)Malin Space Science Systems, San Diego, CA, United States, (8)Southwest Research Institute, San Antonio, United States
John Leif Joergensen1, Finn Eskemann Jørgensen2, Jose M.G. Merayo3, Troelz Denver4, Mathias Benn2, Peter Siegbjoern Joergensen5, John E P Connerney6, Ronald J Oliversen7, Stavros Kotsiaros4, Scott J Bolton8 and Steven Levin9, (1)Technical University of Denmark, Kgs. Lyngby, Denmark, (2)Technical University of Denmark, DTU Space, Lyngby, Denmark, (3)DTU Space, Lyngby, Denmark, (4)Technical University of Denmark, DTU Space, Kgs. Lyngby, Denmark, (5)Technical university of Denamrk, Space, Kgs. Lyngby, Denmark, (6)Space Research Corporation, Annapolis, United States, (7)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (8)Southwest Research Institute, San Antonio, United States, (9)Jet Propulsion Laboratory, Pasadena, United States

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