P082
The Interiors of Jupiter and Saturn in the Era of Juno and Cassini II Posters

Wednesday, 16 December 2020: 04:00-20:59
Poster
Primary Convener:  Kimberly Moore, California Institute of Technology, Pasadena, CA, United States
Conveners:  Sean M Wahl, University of California, Berkeley, Berkeley, CA, United States, David J Stevenson, California Institute of Technology, Pasadena, CA, United States and Scott J Bolton, Southwest Research Institute, San Antonio, TX, United States
Primary Liaison:  Scott J Bolton, Southwest Research Institute, San Antonio, TX, United States
Chairs:  Kimberly Moore, Yale University, New Haven, CT, United States, Sean M Wahl, University of California, Berkeley, Berkeley, CA, United States, David J Stevenson, California Institute of Technology, Pasadena, CA, United States and Scott J Bolton, Southwest Research Institute, San Antonio, TX, United States
OSPA Liaison:  David J Stevenson, California Institute of Technology, Pasadena, CA, United States
 
Cloud and haze activity at Jupiter’s polar regions and zone-belt structure investigated from multispectral and polarimetric observations (768278)
Shuntaro Yokota1, Mitsuteru Sato1, Yukihiro Takahashi2, Seiko Takagi1, Tatsuharu Ono1, Yuki Sato1 and Haruki Sugiyama1, (1)Hokkaido University, Sapporo, Japan, (2)Hokkaido University, Faculty of Science, Sapporo, Japan
 
Constraining the Secular Variation of Saturn’s Magnetic Field. (695682)
Bryce Bolton, Artistic Sciences Inc., San Antonio, United States, Kimberly Moore, Yale University, New Haven, CT, United States, Hao Cao, Harvard, Boston, MA, United States and Jeremy Bloxham, Harvard University, Earth and Planetary Sciences, Cambridge, MA, United States
 
Dynamical tides in the Jovian System as revealed by Juno (712181)
Benjamin Idini and David J Stevenson, California Institute of Technology, Pasadena, CA, United States
 
Updates on Jupiter’s gravity from the latest Juno data (729324)
Daniele Durante1, Virginia Notaro1, Paolo Racioppa2, Luciano Iess2, Marzia Parisi3, Dustin Buccino4, William M Folkner4, Marco Zannoni5, Luis Gomez Casajus6, Paolo Tortora5, David J Stevenson7 and Scott J Bolton8, (1)Sapienza University of Rome, Rome, Italy, (2)Sapienza University of Rome, Department of Mechanical and Aerospace Engineering, Rome, Italy, (3)Jet Propulsion Laboratory, Pasadena, CA, United States, (4)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (5)University of Bologna, Department of Industrial Engineering, Bologna, Italy, (6)University of Bologna, Bologna, Italy, (7)California Institute of Technology, Pasadena, CA, United States, (8)Southwest Research Institute, San Antonio, TX, United States
 
The Range of Jupiter's Flow Structures that Fit the Juno Asymmetric Gravity Measurements (742764)
Keren Duer, Eli Galanti and Yohai Kaspi, Weizmann Institute of Science, Rehovot, Israel
 
Jupiter and Saturn are regular rocky planets surrounded by an ice shell that is in turn cloaked by debris from a crash of early planets; looking at evidence in the era of Juno and Cassini (692172)
Sally Seaver, Independent Scientist, Boston, MA, United States
See more of: Planetary Sciences
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