SM013
Magnetosphere of Jupiter: Multiple Views of a Dynamic System

Session ID#: 158087

Session Description:
Jupiter's large and dynamic magnetosphere has been explored extensively over the past seven years by the Juno spacecraft with complementary measurements from Earth-based observatories (e.g., Hubble, Hisaki, Keck, Nustar). As Juno's polar orbit precesses the trajectory crosses the equator closer to Jupiter, passing the orbits of the Galilean satellites and mapping the middle to inner current sheet and plasma disk. Flybys of Ganymede, Europa and, eventually Io, provide opportunities to explore the plasma-moon interactions. The orbit evolution also brings Juno (at perijove) closer to the ionosphere over the northern auroral region as well as (at apojove) potential magnetopause crossings at the nightside southern boundary. This session seeks submissions that address the dynamics of the jovian magnetosphere from the outer boundaries to Jupiter's atmosphere/ionosphere, including analysis of in situ and/or remote observations, theoretical studies and predictions through the Juno extended mission.
Index Terms:

2732 Magnetosphere interactions with satellites and rings [MAGNETOSPHERIC PHYSICS]
2736 Magnetosphere/ionosphere interactions [MAGNETOSPHERIC PHYSICS]
2740 Magnetospheric configuration and dynamics [MAGNETOSPHERIC PHYSICS]
2756 Planetary magnetospheres [MAGNETOSPHERIC PHYSICS]

Primary Convener:  Fran Bagenal, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
Conveners:  Scott J Bolton1, Yasmina M. Martos2,3 and Vincent Hue1, (1)Southwest Research Institute, San Antonio, TX, United States(2)University of MaryLand, College Park, United States(3)NASA Goddard Space Flight Center, Greenbelt, United States
Student/Early Career Convener:  Tristan Weber, Howard University, Physics & Astronomy, Washington, MD, United States; NASA Goddard Space Flight Center, Greenbelt, United States
 
Beta-dependent Constraints on Ion Temperature Anisotropy in Jupiter's Magnetosheath (1046925)
Luke Begley1, Riddhi Bandyopadhyay2, Bennett Maruca3, David J McComas2, Jamey R Szalay2, Frederic Allegrini4, Robert W Ebert5, Daniel J Gershman6, John E P Connerney6 and Scott J Bolton7, (1)Princeton University, Princeton, NJ, United States, (2)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (3)Center for Astrophysics, Berkeley, CA, United States, (4)Southwest Research Institute San Antonio, San Antonio, TX, United States, (5)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, TX, United States, (6)NASA Goddard Space Flight Center, Greenbelt, United States, (7)Southwest Research Institute, San Antonio, TX, United States
 
Cooling of thermal electrons in the Jovian inner magnetosphere due to the solar wind effect: the HISAKI observation (1051428)
Fuminori Tsuchiya1, Go Murakami2, Masato Kagitani3, Kazuo Yoshioka4, Tomoki Kimura5, Hajime Kita6, Atsushi Yamazaki7, Hiroaki Misawa8, Yasumasa Kasaba1 and Ichiro Yoshikawa4, (1)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (2)ISAS-JAXA, Sagamihara, Japan, (3)PPARC, Tohoku University, Sendai, Japan, (4)The University of Tokyo, Tokyo, Japan, (5)Tokyo University of Science, Department of Physics, Graduate School of Science, Tokyo, Japan, (6)Tohoku Institute of Technology, Sendai, Japan, (7)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (8)Tohoku Univ, Sendai, Japan
 
Juno-UVS Background Measurements of the High-Energy Particle Population and Morphology of the Io Plasma Torus (1052231)
Joshua Kammer1, Randy Gladstone1, Thomas K Greathouse1, Maarten H Versteeg1, Vincent Hue1, Rohini Giles1, Jean-Claude M. C. Gerard2, Denis C Grodent2, Bertrand Bonfond2, Scott J Bolton1, John E P Connerney3 and Steven Levin4, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)Jet Propulsion Laboratory, Pasadena, CA, United States
 
Jupiter’s Galactic Cosmic Ray Cutoff Rigidities and Flux (1052770)
Martin B Enghoff1, Jacob Svensmark2, John L Jørgensen3, Matija Herceg3, Stavros Kotsiaros4 and John E P Connerney5, (1)Technical University of Denmark, Space, Kgs. Lyngby, Denmark, (2)University of Oxford, Physics, Oxford, United Kingdom, (3)Technical University of Denmark, DTU Space, Kgs. Lyngby, Denmark, (4)Technical University of Denmark - Space, Kgs. Lyngby, Denmark, (5)Space Research Corporation, Annapolis, United States
 
Long-Lasting Auroral Injections and the Magnetospheric Processes (1054041)
Zhonghua Yao1, Denis C Grodent2, Binzheng Zhang3, Bertrand Bonfond2 and Peter A Delamere4, (1)Chinese Academy of Sciences, Beijing, China, (2)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (3)Dartmouth College, Hanover, United States, (4)University of Alaska Fairbanks, Fairbanks, AK, United States
 
The Jovian Plasma Disk as Observed from Merging Two Juno JADE Datasets (1057160)
Robert J Wilson, University of Colorado at Boulder, Boulder, United States
 
UVS Observations of Jupiter’s Brightest Aurora of the Juno Mission: Perijove 43 (1058390)
Thomas K Greathouse1, Randy Gladstone1, Maarten H Versteeg1, Vincent Hue1, Joshua Kammer1, Scott J Bolton1, Rohini Giles2, John E P Connerney3, Jean-Claude M. C. Gerard4, Denis C Grodent4, Bertrand Bonfond4 and Steven Levin5, (1)Southwest Research Institute, San Antonio, TX, United States, (2)University of Oxford, Oxford, United Kingdom, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (5)Jet Propulsion Laboratory, Pasadena, CA, United States
 
New Outlook of Jupiter’s Radiation Environment from Juno Data-based Model of the Jovian Electron Belts (1063177)
Daniel Santos-Costa1, Scott J Bolton1, Robert J Wilson2, Philip W Valek1, Rob W Ebert3, Frederic Allegrini4, Peter Kollmann5, Barry Mauk6, Insoo Jun7, Henry Berry Garrett8, Randy Gladstone1, Steven Levin9, Heidi N Becker8 and John E P Connerney10, (1)Southwest Research Institute, San Antonio, TX, United States, (2)University of Colorado at Boulder, Boulder, United States, (3)Southwest Research Institute, Space Science and Engineering, San Antonio, TX, United States, (4)Southwest Research Institute San Antonio, San Antonio, TX, United States, (5)The Applied Physics Laboratory, John Hopkins University, Laurel, United States, (6)The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (7)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (8)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (9)Jet Propulsion Laboratory, Pasadena, CA, United States, (10)NASA Goddard Space Flight Center, Greenbelt, United States
 
Measured Particle Flux Levels and their Importance to Ganymede Weathering (1066464)
Chris Paranicas, Johns Hopkins University Applied Physics Laboratory, Laurel, United States, Peter Kollmann, The Applied Physics Laboratory, John Hopkins University, Laurel, United States, Barry Mauk, The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, George B Clark, Catholic University of America, Washington, United States, Jamey R Szalay, Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, Frederic Allegrini, Southwest Research Institute San Antonio, San Antonio, TX, United States, Rob W Ebert, Southwest Research Institute, Space Science and Engineering, San Antonio, TX, United States, Candice J. Hansen, Planetary Science Institute, Tucson, AZ, United States, Jack H Waite Jr, Southwest Research Institute, Space Sciences and Engineering, San Antonio, TX, United States, Lucas Liuzzo, Space Sciences Laboratory, Berkeley, CA, United States and Scott J Bolton, Southwest Research Institute, San Antonio, TX, United States
 
Plasma wave and particle dynamics during interchange events in the Jovian Magnetosphere using Juno observations (1066941)
Alec Daly1, Wen Li1, Qianli Ma2,3, Xiaochen Shen1, Peter H Yoon4 and John Douglas Menietti5, (1)Boston University, Boston, United States, (2)Boston University, Boston, MA, United States, (3)University of California Los Angeles, Atmospheric and Oceanic Sciences, Los Angeles, United States, (4)Univ Maryland, College Park, MD, United States, (5)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States
 
Axial Asymmetry in Jovian Magnetopause Reconnection (1077059)
Junjie Chen, University of Hong Kong, Department of Earth Sciences, Hong Kong, Hong Kong, Binzheng Zhang, Dartmouth College, Hanover, United States, Dong Lin, NCAR, Boulder, United States, Peter A Delamere, University of Alaska Fairbanks, Fairbanks, AK, United States, Zhonghua Yao, Chinese Academy of Sciences, Beijing, China, Oliver Brambles, Thayer School of Engineering, Hanover, United States, Kareem Sorathia, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Viacheslav G Merkin, The Johns Hopkins University, APL, Laurel, United States and John Lyon, Dartmouth College, Hanover, NH, United States
 
Electron Densities over Jupiter’s Polar Cap and Implications for Auroral Acceleration (1077944)
Ali H Sulaiman1, Sadie Elliott2, Robert L Lysak1, Frederic Allegrini3, William S Kurth4, George B Hospodarsky4, Ondrej Santolik5, George B Clark6, Barry Mauk7 and Scott J Bolton8, (1)University of Minnesota, School of Physics and Astronomy, Minneapolis, United States, (2)University of Minnesota Twin Cities, School of Physics and Astronomy, Minneapolis, United States, (3)Southwest Research Institute San Antonio, San Antonio, TX, United States, (4)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (5)IAP Prague, Praha 4, Czech Republic, (6)Catholic University of America, Washington, United States, (7)The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (8)Southwest Research Institute, San Antonio, TX, United States
 
Status on the Recovery of Voyager Plasma Electron Observations at Jupiter (1091347)
Edward C Sittler Jr1, William R Paterson1, Daniel J Gershman2, David G Simpson3 and John F Cooper4, (1)NASA Goddard Space Flight Center, Geospace Physics Laboratory, Greenbelt, MD, United States, (2)NASA Goddard Space Flight Center, Greenbelt, United States, (3)NASA Goddard Space Flight Ctr, Greenbelt, MD, United States, (4)NASA Goddard Space Flight Center (Emeritus), Heliospheric Physics Laboratory, Greenbelt, MD, United States
 
Characteristics of dispersive Alfvén waves inferred from the newly developed magnetospheric plasma distribution model (1101869)
Koseki Saito1, Yuto Katoh1, Tomoki Kimura2, Yohei Kawazura3, Masahiro Kitahara1 and Atsushi Kumamoto1, (1)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (2)Tokyo University of Science, Department of Physics, Graduate School of Science, Tokyo, Japan, (3)Tohoku University, The Frontier Research Institute for Interdisciplinary Sciences, Sendai, Japan
 
Dynamic Jovian Magnetosphere Responses to Enhanced Solar Wind Ram Pressure (1104187)
Enhao Feng1, Binzheng Zhang2, Zhonghua Yao3, Peter A Delamere4, Zheng Zhiqi2, Oliver Brambles5, Shengyi Ye6 and Kareem Sorathia7, (1)University of Hong Kong, Hong Kong, HONG KONG, (2)University of Hong Kong, Department of Earth Sciences, Hong Kong, Hong Kong, (3)Chinese Academy of Sciences, Beijing, China, (4)University of Alaska Fairbanks, Fairbanks, AK, United States, (5)Preston UK, Preston, United Kingdom, (6)Southern University of Science and Technology, Department of Earth and Space Sciences, Shenzhen, China, (7)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
 
Distributions of Ions Observed In Situ in the Topside, Equatorial Jovian Ionosphere (1109279)
Philip W Valek1, Frederic Allegrini2, Fragn Bagenal3, Scott J Bolton1, John E P Connerney4, Vincent J Dols5, Robert W Ebert6, William S Kurth7, Jamey R Szalay8, Hunter Waite Jr9 and Robert J Wilson10, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute San Antonio, San Antonio, TX, United States, (3)University of Colorado Boulder - LASP, Boulder, United States, (4)NASA Goddard Space Flight Center, Greenbelt, United States, (5)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (6)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, TX, United States, (7)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (8)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (9)Southwest Research Institute, San Antonio, United States, (10)University of Colorado at Boulder, Boulder, United States
 
Tracking Jupiter’s Secondary Oval’s Response to Injections. (1110648)
Diego Moral Pombo, Lancaster University, Physics Department, Glasgow, United Kingdom, Sarah Victoria Badman, Lancaster University, Physics Department, Lancaster, United Kingdom, Jonathan D Nichols, University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, Denis C Grodent, Université de Liège, LPAP - STAR Institute, Liege, Belgium and Dale Weigt, Dublin Institute for Advance Studies, Dublin, Ireland
 
Observations of Jupiter’s Dusk Magnetopause at High Southern Latitude: Implications for 3-D Magnetosphere Structure and Solar Wind Interactions (1114054)
Robert W Ebert1,2, Frederic Allegrini3, Fran Bagenal4, Riddhi Bandyopadhyay5, Scott J Bolton6, John E P Connerney7, William S Kurth8, Corentin Louis9, David J McComas10, Jake Montgomery6,11, Jamey R Szalay10, Philip W Valek6 and Robert J Wilson12, (1)University of Texas at San Antonio, San Antonio, United States, (2)Southwest Research Institute, San Antonio, United States, (3)Southwest Research Institute San Antonio, San Antonio, TX, United States, (4)Univ Colorado, Boulder, United States, (5)Princeton University, Department of Astrophysics, Princeton, NJ, United States, (6)Southwest Research Institute, San Antonio, TX, United States, (7)NASA Goddard Space Flight Center, Greenbelt, United States, (8)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (9)Observatoire de Paris, PSL, CNRS, Sorbonne Univ., UMPC, LESIA, Meudon, France, (10)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (11)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (12)University of Colorado at Boulder, Boulder, United States
 
Dynamics of Field-Aligned Currents and Parallel Electric Fields over Jupiter’s Polar Caps (1115175)
Robert L Lysak1, William S Kurth2, Ali H Sulaiman1, Sadie Elliott3, Yan Song4, George B Clark5, Barry Mauk6 and Fran Bagenal7, (1)University of Minnesota, School of Physics and Astronomy, Minneapolis, United States, (2)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (3)University of Minnesota Twin Cities, School of Physics and Astronomy, Minneapolis, United States, (4)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (6)The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (7)Univ Colorado, Boulder, United States
 
Synchrotron Observations From The Juno Microwave Radiometer at Jupiter (1115710)
Steven Levin, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and The Juno MWR Team
 
Multifluid Simulations of Kinetic Alfven Wave Resonances in Jovian and Terrestrial Magnetospheres (1116216)
Aaron F F West, University of Minnesota Twin Cities, Physics, Minneapolis, United States and Robert L Lysak, University of Minnesota, School of Physics and Astronomy, Minneapolis, United States
 
Investigating the Occurrence of Kelvin-Helmholtz Instabilities at Jupiter’s Dawn Magnetopause (1116746)
Jake Montgomery1, Robert Ebert2, Frederic Allegrini3, Fran Bagenal4, Scott J Bolton1, Gina A DiBraccio5, Stephen A Fuselier1 and Robert J Wilson6, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, United States, (3)Southwest Research Institute San Antonio, San Antonio, TX, United States, (4)Univ Colorado, Boulder, United States, (5)University of Michigan, Ann Arbor, United States, (6)University of Colorado at Boulder, Boulder, United States
 
Juno Observations of Jovian Long Dispersion Lightning Whistlers associated with the Io torus (1121933)
George B Hospodarsky1, William S Kurth1, Masafumi Imai2, Ivana Kolmasova3, Ondrej Santolik3, John E P Connerney4 and Scott J Bolton5, (1)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (2)National Institute of Technology, Department of Electrical Engineering and Information Scienc, Ehime, Japan, (3)IAP Prague, Praha 4, Czech Republic, (4)NASA Goddard Space Flight Center, Greenbelt, United States, (5)Southwest Research Institute, San Antonio, TX, United States
 
A Survey of Ultra-Low Frequency Waves in Jupiter's Middle Magnetosphere (1126082)
Frank J Crary, University of Colorado at Boulder, Boulder, CO, United States
 
Spatial and temporal variations in the CH4 homopause altitude at Jupiter’s mid-to-high latitudes (1131288)
James Andrew Sinclair1, Thomas K Greathouse2, Rohini Giles3, Matthew Richter4, Curtis deWitt5, Julianne I Moses6, Vincent Hue2, Catherine Deng7, Glenn Orton8, Leigh N. Fletcher9 and Patrick GJ Irwin10, (1)NASA Jet Propulsion Laboratory, Pasadena, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)Southwest Research Institute, San Antonio, United States, (4)University of California Davis, Davis, CA, United States, (5)NASA Ames Research Center, Moffett Field, United States, (6)Space Science Institute, Seabrook, TX, United States, (7)California Institute of Technology, Pasadena, United States, (8)Jet Propulsion Laboratory, Pasadena, CA, United States, (9)University of Leicester, Leicester, United Kingdom, (10)University of Oxford, Oxford, United Kingdom
 
Magnetospheric origin of Jovian auroral dawn storms (1142882)
Binzheng Zhang1, Peter A Delamere2, Zhonghua Yao3, William Lotko4, Kareem Sorathia5, Oliver Brambles6, Bertrand Bonfond7, Denis C Grodent7 and John Lyon8, (1)University of Hong Kong, Department of Earth Sciences, Hong Kong, Hong Kong, (2)University of Alaska Fairbanks, Fairbanks, AK, United States, (3)Chinese Academy of Sciences, Beijing, China, (4)Dartmouth College, Thayer School of Engineering, Hanover, United States, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (6)Thayer School of Engineering, Hanover, United States, (7)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (8)Dartmouth College, Hanover, NH, United States
 
Structure and dynamics of Jupiter’s dawnside magnetosphere: model/data comparisons (1166619)
Peter A Delamere1, Peter A Damiano1, Blake Mino1, Andrew Schok1, Xuanye Ma2, Jay Johnson3, Binzheng Zhang4, Kareem Sorathia5, Anthony Sciola6, Simon Wing7, George B Clark8, Robert J Wilson9 and Fran Bagenal10, (1)University of Alaska Fairbanks, Fairbanks, AK, United States, (2)Embry-Riddle Aeronautical University, Physical Sciences -- Center for Space and Atmospheric Research, Daytona Beach, United States, (3)Andrews University, Berrien Springs, MI, United States, (4)University of Hong Kong, Department of Earth Sciences, Hong Kong, Hong Kong, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (6)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (7)The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (8)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (9)University of Colorado at Boulder, Boulder, United States, (10)Univ Colorado, Boulder, United States
 
The Generation of Radial Outflow Velocity in the Magnetosphere of Jupiter and the Coupling with Turbulent Heating (1170184)
Chung-Sang Ng1, Peter A Delamere2 and Peter A Damiano2, (1)University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States, (2)University of Alaska Fairbanks, Fairbanks, AK, United States
 
Find Your Favorite Io Volcanic Enhancement! A Global View of the Jovian Magnetosphere During the Juno Mission as Recorded by PSI's Io Input/Output Observatory (IoIO) (1181592)
Jeffrey P Morgenthaler1, Carl Schmidt2, Max Marconi3, Marissa F. Vogt2 and Nicholas McCord Schneider4, (1)Planetary Science Institute, Fort Kent, United States, (2)Boston University, Center for Space Physics, Boston, United States, (3)Prisma Basic Research, Niagara Falls, NY, United States, (4)Univ Colorado, Boulder, United States
 
Low Latitude Trapped Jovian Electrons Measured by Juno/JADE (1198841)
Frederic Allegrini1, Peter Kollmann2, Robert W Ebert3, Jamey R Szalay4, Fragn Bagenal5, Philippe Louarn6, David J McComas4, Angele Pontoni1, Philip W Valek1, Robert J Wilson7, William S Kurth8, Scott J Bolton1 and John E P Connerney9, (1)Southwest Research Institute, San Antonio, TX, United States, (2)The Applied Physics Laboratory, John Hopkins University, Laurel, United States, (3)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, TX, United States, (4)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (5)University of Colorado Boulder - LASP, Boulder, United States, (6)IRAP, CNRS, Toulouse, France, (7)University of Colorado at Boulder, Boulder, United States, (8)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (9)NASA Goddard Space Flight Center, Greenbelt, United States
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