SM23G:
Our Evolving Understanding of Auroral Processes and Magnetosphere Dynamics at Jupiter Through Juno and Earth-Based Observations II Posters


Submit an Abstract to this Session


Session ID#: 51758

Session Description:
Our view and understanding of Jupiter’s auroras and magnetosphere are ever-changing as Juno continues to explore these regions in situ with coordinated efforts from Earth-based observatories such as Hubble, Hisaki, Keck, etc. These new measurements have illuminated new and exciting discoveries that are challenging our theoretical ideas. This session seeks submissions covering new observations and interpretations, theories, and models of Jupiter’s auroral regions, magnetosphere and/or ionosphere and their connection. Specifically, this session will cover the following topics: observation and theory of auroral acceleration including wave-particle interactions; auroral phenomenology, magnetosphere-ionosphere coupling; plasma sheet dynamics; outer boundary structure and dynamics, and particle acceleration and transport. This session aims to share the most recent observations and ideas regarding Jupiter’s magnetosphere, while providing a forum that takes a multidisciplinary approach to furthering our knowledge of this system.
Primary Convener:  Robert W Ebert, Southwest Research Institute, San Antonio, TX, United States
Conveners:  Scott J Bolton, Southwest Research Institute, San Antonio, United States, George B Clark, The Johns Hopkins University Applied Physics Laboratory, Laurel, United States and Masafumi Imai, University of Iowa, Physics and Astronomy, Iowa City, IA, United States
Primary Liaison:  Robert W Ebert, University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States
Chairs:  George B Clark, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Masafumi Imai, University of Iowa, Physics and Astronomy, Iowa City, IA, United States
OSPA Liaison:  Robert W Ebert, University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States
Co-Organized with:
SPA-Magnetospheric Physics, and Planetary Sciences

Cross-Listed:
  • P - Planetary Sciences

Proposed Co-Organized Session with:
  • P - Planetary Sciences
Index Terms:

2704 Auroral phenomena [MAGNETOSPHERIC PHYSICS]
2756 Planetary magnetospheres [MAGNETOSPHERIC PHYSICS]
5719 Interactions with particles and fields [PLANETARY SCIENCES: FLUID PLANETS]
6220 Jupiter [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Abstracts Submitted to this Session:

Jupiter X-Ray Aurora: Evidence from Juno (353060)
Stephen Jeffrey Houston1, Thomas Cravens2, David R Schultz3, Barry Mauk4, Dennis K Haggerty5, William Dunn6 and Abigail M Rymer4, (1)Applied Physics Laboratory Johns Hopkins, Laurel, KS, United States, (2)University of Kansas, Physics and Astronomy, Lawrence, KS, United States, (3)Northern Arizona State, Flagstaff, AZ, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)Johns Hopkins Univ, Laurel, MD, United States, (6)University College London, Department of Phyics and Astronomy, London, United Kingdom
Probing Ion Precipitation at Jupiter’s Poles Through Dynamic X-ray Spectra (406704)
William Dunn1, Graziella Branduardi-Raymont2, Jan Uwe Ness3, Randy Gladstone4, Abigail M Rymer5, Stephen Jeffrey Houston6, Thomas Cravens7, Caitriona Mary Jackman8, Ralph Kraft9, Licia C Ray10, Zhonghua Yao11, Nicholas A Achilleos12, Denis C Grodent13, James Andrew Sinclair14, Ronald Elsner15, Chris Paranicas5, George B Clark5, Barry Mauk5 and Dennis K Haggerty16, (1)University College London, Department of Phyics and Astronomy, London, United Kingdom, (2)University College London, Mullard Space Science Laboratory, London, United Kingdom, (3)European Space Agency, Villanueva De La Can, Spain, (4)Southwest Research Institute, San Antonio, United States, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (6)Applied Physics Laboratory Johns Hopkins, Laurel, KS, United States, (7)University of Kansas, Physics and Astronomy, Lawrence, KS, United States, (8)University of Southampton, Southampton, United Kingdom, (9)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (10)University College London, London, United Kingdom, (11)Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China, (12)University College London, Department of Physics and Astronomy, London, United Kingdom, (13)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (14)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (15)NASA Marshall Space Flight Center, Huntsville, AL, United States, (16)Johns Hopkins Univ, Laurel, MD, United States
Jupiter’s Auroral Morphology: X-Ray and UV Emission Associated with Energetic Particles Observed by Juno-JEDI. (407781)
Abigail M Rymer1, Randy Gladstone2, William Dunn3, Dennis K Haggerty4, Barry Mauk5, Peter Kollmann6, Scott J Bolton2, John E P Connerney7, Masafumi Imai8, Graziella Branduardi-Raymont9 and Tom Stallard10, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (2)Southwest Research Institute, San Antonio, United States, (3)University College London, Department of Physics and Astronomy, London, United Kingdom, (4)Johns Hopkins Univ, Laurel, MD, United States, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (6)The Applied Physics Laboratory, John Hopkins University, Laurel, United States, (7)Space Research Corporation, Annapolis, United States, (8)Kyoto University, Kyoto, Japan, (9)University College London, Mullard Space Science Laboratory, London, United Kingdom, (10)University of Leicester, Leicester, United Kingdom
Radial Transport in Jupiter's Magnetosphere (375218)
Fran Bagenal, University of Colorado at Boulder, Boulder, CO, United States, Robert J Wilson, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, Ezra Huscher, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, Frederic Allegrini, Southwest Research Institute, San Antonio, United States, John E P Connerney, Space Research Corporation, Annapolis, United States, Lori Spalsbury, ADNET Systems Inc. Greenbelt, Greenbelt, MD, United States and Juno Science Team
The Jovian Magnetodisc Azimuthal and Radial Fields Mapped by the Juno Spacecraft (400412)
Lori Spalsbury, Space Research Corporation, Annapolis, MD, United States, John E P Connerney, Space Research Corporation, Annapolis, United States, Daniel J Gershman, NASA Goddard Space Flight Center, Greenbelt, United States, Marissa F. Vogt, Boston University, Boston, United States, Fran Bagenal, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, Scott J Bolton, Southwest Research Institute, San Antonio, United States and Steven Levin, Jet Propulsion Laboratory, Pasadena, United States
Latitudinal and Radial Dependence of Plasma Sheet Ion Properties at Jupiter: Juno JADE-I Observations (412283)
Thomas K Kim1,2, Robert W Ebert3, Philip W Valek2, Frederic Allegrini2, David J McComas2,4, Fran Bagenal5, George Livadiotis2, Michelle F Thomsen6, Robert J Wilson5, George B Clark7, John E P Connerney8, Peter Kollmann9, William S Kurth10, Barry Mauk9, Scott J Bolton11 and Steven Levin12, (1)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (4)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (5)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (6)Planetary Science Institute, Tuscon, AZ, United States, (7)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (8)Space Research Corporation, Annapolis, United States, (9)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (10)University of Iowa, Iowa City, IA, United States, (11)Southwest Research Institute, San Antonio, United States, (12)Jet Propulsion Laboratory, Pasadena, United States
Variability in the Io Plasma Torus Seen by Juno Radio Occultations (438966)
Phillip H Phipps, Boston University, Boston, MA, United States, Paul Withers, Boston University, Boston, United States, Dustin Buccino, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, Yu-Ming Yang, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Parker C Hinton, Department of Astrophysical and Planetary Sciences, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States and Fran Bagenal, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
A 2-D Io Torus Physical Chemistry Model that Combines Latitudinal and Radial Variations (445334)
Edward Gregory Nerney, PhD and Fran Bagenal, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
Energetic charged particle characteristics of Jupiter’s middle-to-outer magnetosphere: Observations from Juno/JEDI (452873)
George B Clark1, Barry Mauk2, Chris Paranicas2, Dennis K Haggerty3, Peter Kollmann4, Abigail M Rymer2, Frederic Allegrini5, Scott J Bolton5, Emma J Bunce6, John E P Connerney7, Robert W Ebert8, Daniel J Gershman9, Steven Levin10, William S Kurth11, David J McComas12, Elias Roussos13, Joachim Saur14, Michelle F Thomsen15 and Marissa F. Vogt16, (1)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (3)Johns Hopkins Univ, Laurel, MD, United States, (4)The Applied Physics Laboratory, John Hopkins University, Laurel, United States, (5)Southwest Research Institute, San Antonio, United States, (6)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (7)Space Research Corporation, Annapolis, United States, (8)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (9)NASA Goddard Space Flight Center, Greenbelt, United States, (10)Jet Propulsion Laboratory, Pasadena, United States, (11)University of Iowa, Iowa City, IA, United States, (12)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (13)Max Planck Institute for Solar System Research, Göttingen, Germany, (14)University of Cologne, Cologne, Germany, (15)Planetary Science Institute, Tuscon, AZ, United States, (16)Boston University, Boston, United States
Magnetotail Reconnection at Jupiter: A survey of magnetic field and plasma flow signatures observed by Juno (457873)
Marissa F. Vogt1, Michelle F Thomsen2, Robert W Ebert3, Robert J Wilson4, Frederic Allegrini5, John E P Connerney6, Gina A DiBraccio7, Daniel J Gershman8, George B Clark9, Chris Paranicas9, William S Kurth10 and Philip W Valek5, (1)Boston University, Center for Space Physics, Boston, United States, (2)Planetary Science Institute, Tuscon, AZ, United States, (3)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (4)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (5)Southwest Research Institute, San Antonio, United States, (6)Space Research Corporation, Annapolis, United States, (7)University of Michigan, Ann Arbor, United States, (8)NASA Goddard Space Flight Center, Greenbelt, United States, (9)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (10)University of Iowa, Iowa City, IA, United States
Jupiter’s Dawn Magnetosheath, Magnetopause, and Polar Flattening as Measured by Juno (467253)
Drake A Ranquist1, Fran Bagenal2, Robert J Wilson2, George B Hospodarsky3, Frederic Allegrini4, Philip W Valek4, John E P Connerney5 and William S Kurth6, (1)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (2)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (3)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (4)Southwest Research Institute, San Antonio, United States, (5)Space Research Corporation, Annapolis, United States, (6)University of Iowa, Iowa City, IA, United States
Rider on the Storm: Juno-UVS Radiation Measurements of an Auroral Dawn Storm (364119)
Joshua Kammer1, Randy Gladstone2, Thomas K Greathouse2, Vincent Hue1, Maarten Versteeg1, Bertrand Bonfond3, Denis C Grodent3, Jean-Claude M. C. Gerard3, Heidi N Becker4, Scott J Bolton2, John E P Connerney5 and Steven Levin6, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, United States, (3)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (4)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (5)Space Research Corporation, Annapolis, United States, (6)Jet Propulsion Laboratory, Pasadena, United States
Flying through a Dawn Storm : an analysis of Juno-UVS images during PJ11 (367647)
Bertrand Bonfond1, Randy Gladstone2, Denis C Grodent1, Zhonghua Yao3, Jean-Claude M. C. Gerard1, Joshua Kammer4, Vincent Hue4, Thomas K Greathouse2, Maarten Versteeg4, William S Kurth5, Philippe Louarn6, George B Hospodarsky7, Masafumi Imai8, John E P Connerney9, Daniel J Gershman10, Stavros Kotsiaros11, Alberto Adriani12, Barry Mauk13, Frederic Allegrini2, Steven Levin14 and Scott J Bolton2, (1)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (2)Southwest Research Institute, San Antonio, United States, (3)Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China, (4)Southwest Research Institute, San Antonio, TX, United States, (5)University of Iowa, Iowa City, IA, United States, (6)CNRS - Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (7)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (8)Kyoto University, Kyoto, Japan, (9)Space Research Corporation, Annapolis, United States, (10)NASA Goddard Space Flight Center, Greenbelt, United States, (11)Technical University of Denmark, DTU Space, Kgs. Lyngby, Denmark, (12)INAF-IAPS, Rome, Italy, (13)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (14)Jet Propulsion Laboratory, Pasadena, United States
Juno-UVS observation of the Io footprint during eclipse (393095)
Vincent Hue1, Bertrand Bonfond2, Michael Wayne Davis1, Jean-Claude M. C. Gerard2, Randy Gladstone3, Thomas K Greathouse3, Denis C Grodent2, Joshua Kammer3, Lorenz Roth4, Joachim Saur5, Maarten Versteeg1, Scott J Bolton3, John E P Connerney6 and Steven Levin7, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (3)Southwest Research Institute, San Antonio, United States, (4)KTH Royal Institute of Technology, Division of Space and Plasma Physics, School of Electrical Engineering, Stockholm, Sweden, (5)University of Cologne, Cologne, Germany, (6)Space Research Corporation, Annapolis, United States, (7)Jet Propulsion Laboratory, Pasadena, United States
Ultraviolet aurora’s response to solar wind measured with Hisaki and Juno (434552)
Hajime Kita1, Tomoki Kimura2, Chihiro Tao3, Fuminori Tsuchiya4, Go Murakami5, Atsushi Yamazaki6, Robert W Ebert7, Philip W Valek8, George B Clark9, John E P Connerney10, Randy Gladstone8, Kazuo Yoshioka11, Yasumasa Kasaba12, Ichiro Yoshikawa11 and Masaki Fujimoto6, (1)ISAS/JAXA, Sagamihara, Japan, (2)Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai, Japan, (3)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (4)Tohoku University, Sendai, Japan, (5)ISAS-JAXA, Sagamihara, Japan, (6)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (7)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (8)Southwest Research Institute, San Antonio, United States, (9)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (10)Space Research Corporation, Annapolis, United States, (11)The University of Tokyo, Tokyo, Japan, (12)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan
Jupiter’s magnetic field and source location of decametric radio emissions observed by Juno (446252)
Yasmina M. Martos, NASA Goddard Space Flight Center, Greenbelt, United States; University of Maryland College Park, College Park, United States, Masafumi Imai, University of Iowa, Physics and Astronomy, Iowa City, IA, United States, John E P Connerney, Space Research Corporation, Annapolis, United States and Stavros Kotsiaros, NASA Goddard Space Flight Center, Greenbelt, MD, United States; University of Maryland College Park, College Park, MD, United States
Juno/Waves Observations of Intense Broadband Electromagnetic Emissions below the Ion Cyclotron Frequency (393711)
Ali H Sulaiman1, William S Kurth2, George B Hospodarsky3, John E P Connerney4, Frederic Allegrini5 and Scott J Bolton5, (1)University of Minnesota, School of Physics and Astronomy, Minneapolis, United States, (2)University of Iowa, Iowa City, IA, United States, (3)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (4)Space Research Corporation, Annapolis, United States, (5)Southwest Research Institute, San Antonio, United States
On the generation of the jovian radio emissions by electron conics: linear amplification and saturation processes (353791)
Philippe Louarn1, William S Kurth2, Frederic Allegrini3, David J McComas4, Corentin Louis5, Nicolas André6, Philip W Valek3, Fran Bagenal7, Jamey R Szalay8, Scott J Bolton3, Robert W Ebert9, Masafumi Imai10 and Robert J Wilson7, (1)IRAP, Toulouse, France, (2)University of Iowa, Iowa City, IA, United States, (3)Southwest Research Institute, San Antonio, United States, (4)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (5)Observatoire de Paris, PSL, CNRS, Sorbonne Univ., UMPC, LESIA, Meudon, France, (6)IRAP, CNRS, Toulouse, France, (7)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (8)University of Colorado at Boulder, Physics, Boulder, United States, (9)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (10)Kyoto University, Kyoto, Japan
A Source of Jovian Broadband Kilometric Radiation Associated with a Dawn Storm Aurora (364381)
William S Kurth1, Philippe Louarn2, Frederic Allegrini3, Barry Mauk4, Bertrand Bonfond5, Randy Gladstone3, Denis C Grodent5, Alberto Adriani6, Corentin Louis7, Masafumi Imai1, George B Hospodarsky1, John E P Connerney8 and Scott J Bolton3, (1)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (2)CNRS - Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (3)Southwest Research Institute, San Antonio, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (6)INAF-IAPS, Rome, Italy, (7)Observatoire de Paris, PSL, CNRS, Sorbonne Univ., UMPC, LESIA, Meudon, France, (8)Space Research Corporation, Annapolis, United States
Dispersive scale Alfven waves and broadband electron energization in the Jovian magnetosphere (423896)
Peter A Damiano1, Peter A Delamere2, Blake Hughes Stauffer1 and Jay Johnson3, (1)University of Alaska Fairbanks, Fairbanks, AK, United States, (2)University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States, (3)Andrews University, Berrien Springs, United States
Energization Mechanisms Leading to Vertical Ion Transport in Jupiter’s Auroral Region Ionosphere (412305)
Katherine Garcia-Sage, NASA Goddard Space Flight Center, Community Coordinated Modeling Center, Greenbelt, MD, United States, Alex Glocer, NASA/GSFC, Greenbelt, United States, Jared Micheal Bell, NASA Goddard Space Flight Center, Code 675, Greenbelt, MD, United States and Sophia Singh, University of Southern California, Los Angeles, United States
A Dynamical Theory of High Energy Discrete Auroral Acceleration by Alfvenic Electrostatic Plasma Structures at Earth and Jupiter (398492)
Yan Song, University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States and Robert L Lysak, University of Minnesota, School of Physics and Astronomy, Minneapolis, United States
Obstruction of Low Energy Electron Trajectories to JADE-E Due to Jupiter’s Strong Magnetic Field and its Effect on Pitch Angle Measurements (415112)
Juan Rafael Munoz Jr1, Frederic Allegrini2, Rob W Ebert2, David J McComas3, Fran Bagenal4, Robert J Wilson5, Philip W Valek2, Philippe Louarn6 and Thomas K Kim1, (1)University of Texas at San Antonio, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, United States, (3)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (4)University of Colorado at Boulder, Boulder, CO, United States, (5)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (6)CNRS - Institut de Recherche en Astrophysique et Planétologie, Toulouse, France

See more of: SPA-Magnetospheric Physics