SM33C:
Magnetospheres in the Outer Solar System II Posters

Submit an Abstract to this Session



Session ID#: 22654

Session Description:
Magnetospheres in the outer solar system have unique characteristics due to factors such as satellite sources of plasma, circumplanetary neutral tori, and rapid planetary rotation. This session invites submissions covering the structure and dynamics of the magnetospheres of the giant planets (Jupiter, Saturn, Uranus and Neptune) as well as Ganymede’s magnetosphere. Papers on magnetospheric and auroral processes including magnetosphere-ionosphere coupling, plasma transport, tail dynamics, rotational modulations, magnetospheric boundaries, and the role of the solar wind are consistent with our themes. We particularly encourage submissions that compare the giant planet magnetospheres to one another, or compare them to those of terrestrial planets. The session will be an ideal forum for the discussion of recent advances in our understanding of all these systems enabled by in-situ and remote observations as well as theoretical and numerical modeling, and relevant to a number of ongoing and future planetary missions to the outer solar system.
Primary Convener:  Xianzhe Jia, University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States
Conveners:  Chris Paranicas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and George B Hospodarsky, University of Iowa, Iowa City, IA, United States
Chairs:  Chris Paranicas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Xianzhe Jia, University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States
OSPA Liaison:  Xianzhe Jia, University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States
Co-Organized with:
SPA-Magnetospheric Physics, and Planetary Sciences

Cross-Listed:
  • P - Planetary Sciences
Index Terms:

5719 Interactions with particles and fields [PLANETARY SCIENCES: FLUID PLANETS]
5737 Magnetospheres [PLANETARY SCIENCES: FLUID PLANETS]
6299 General or miscellaneous [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
7899 General or miscellaneous [SPACE PLASMA PHYSICS]

Abstracts Submitted to this Session:

Polar Plasma at Ganymede: Ionospheric outflow and discovery of the plasma sheet (225220)
Glyn Collinson1, William R Paterson2, John C Dorelli1, Alex Glocer3, Menelaos Sarantos4, Robert J Wilson5 and Christopher Bard2, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (3)NASA Goddard Space Flight Center, Heliophysics Division, Greenbelt, United States, (4)NASA Goddard Space Flight Center, Greenbelt, United States, (5)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
Ionospheric energization, field-aligned transport, and escape at Jupiter (244333)
Alex Glocer, NASA Goddard Space Flight Center, Heliophysics Division, Greenbelt, United States, Katherine Garcia-Sage, Catholic University of America, Washington, DC, United States and Jared Micheal Bell, NASA Goddard Space Flight Center, Code 675, Greenbelt, MD, United States
Magnetosphere - Ionosphere - Thermosphere (MIT) Coupling at Jupiter (250696)
Japheth Nesta Yates, European Space Agency, Villanueva De La Can, Spain, Licia C Ray, Lancaster University, Lancaster, United Kingdom and Nicholas A Achilleos, University College London, Department of Physics and Astronomy, London, United Kingdom
A 4D model of the Io plasma torus (256065)
Parker C Hinton, Department of Astrophysical and Planetary Sciences, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, Fran Bagenal, University of Colorado at Boulder, Boulder, CO, United States and Kaleb Michael Bodisch, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
Variations of System IV period of the sulfur ions in the Io torus for the volcanic event in 2015 observed by the HISAKI/EXCEED (281285)
Arakawa Ryo1, Hiroaki Misawa2, Fuminori Tsuchiya3, Masato Kagitani4, Kazuo Yoshioka5, Ichiro Yoshikawa6, Tomoki Kimura7, Go Murakami8 and Atsushi Yamazaki8, (1)Tohoku University, Sendai, Japan, (2)Tohoku Univ, Sendai, Japan, (3)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (4)PPARC, Tohoku University, Sendai, Japan, (5)ISAS/JAXA, Kanagawa, Japan, (6)The University of Tokyo, Tokyo, Japan, (7)Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai, Japan, (8)ISAS/JAXA, Sagamihara, Kanagawa, Japan
Modeling the Evolution of the System IV Period of the Io Torus (284974)
Drew A Coffin, University of Alaska Fairbanks, Fairbanks, AK, United States and Peter A Delamere, University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States
Constraining Plasma Conditions of the IPT via Spectral Analysis of UV & Visible Emissions and Comparing with a Physical Chemistry Model (291735)
Edward Gregory Nerney, PhD, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, Fran Bagenal, University of Colorado at Boulder, Boulder, CO, United States, Kazuo Yoshioka, ISAS/JAXA, Kanagawa, Japan and Carl Schmidt, LATMOS, Paris, France
Radial and azimuthal distribution of Io’s oxygen neutral cloud observed by Hisaki/EXCEED (295502)
Ryoichi Koga1, Fuminori Tsuchiya2, Masato Kagitani3, Takeshi Sakanoi1, Mizuki Yoneda3, Ichiro Yoshikawa4, Kazuo Yoshioka5, Go Murakami6, Atsushi Yamazaki6, Tomoki Kimura7 and Howard Todd Smith8, (1)PPARC, Tohoku University, Sendai, Japan, (2)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (3)Tohoku University, Sendai, Japan, (4)The University of Tokyo, Tokyo, Japan, (5)University of Tokyo, Bunkyo-ku, Japan, (6)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (7)RIKEN, Wako, Japan, (8)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States
Effect of plasma density around Io on local electron heating in the Io plasma torus (297343)
Fuminori Tsuchiya1, Kazuo Yoshioka2, Masato Kagitani1, Tomoki Kimura3, Go Murakami4, Atsushi Yamazaki5, Hiroaki Misawa1, Yasumasa Kasaba6, Ichiro Yoshikawa7, Takeshi Sakanoi8, Ryoichi Koga8, Arakawa Ryo1, Fumiharu Suzuki7 and Reina Hikida7, (1)Tohoku University, Sendai, Japan, (2)University of Tokyo, Graduate School of Frontier Science, Bunkyo-ku, Japan, (3)Japan Aerospace Exploration Agency, Kanagawa, Japan, (4)ISAS-JAXA, Sagamihara, Japan, (5)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (6)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (7)The University of Tokyo, Tokyo, Japan, (8)PPARC, Tohoku University, Sendai, Japan
Jupiter radiation measurements from enhanced Galileo/EPD data for NASA’s PDS archive (226643)
Peter Kollmann1, Daniel Smith2, Jon Duane Vandegriff2, Chris Paranicas1 and Zoe H. Lee-Payne3, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (3)Aberystwyth University, Aberystwyth, United Kingdom
MHD simulations of the interaction of the Solar Wind with fast-rotating planetary magnetospheres using a time-dependant background/residual decomposition of the magnetic field (231668)
Léa Sophie Griton, IRAP, Université Toulouse III—Paul Sabatier, CNRS, CNES, Toulouse, France, Filippo G E Pantellini, CNRS, Observatoire de Paris, LESIA, Meudon, France and Michel Moncuquet, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, LESIA, Meudon, France
Plasma circulation in Jupiter's magnetosphere (292737)
Emmanuel Chané, Katholieke Universiteit Leuven, Leuven, Belgium
Influence of the solar wind and IMF on Jupiter’s magnetosphere: Results from global MHD simulations (236261)
Yash Sarkango1, Xianzhe Jia2, Gabor Toth3 and Kenneth C Hansen1, (1)University of Michigan, Ann Arbor, MI, United States, (2)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
Rotation of the interplanetary magnetic field in the Jovian and Kronian magnetosheaths (273953)
Iris Daniela Ponce, Organization Not Listed, Washington, DC, United States and Mariel Meier, Oglethorpe University, Physics, Atlanta, GA, United States
Investigation of Magnetic Reconnection Suppression at Saturn’s Magnetopause (225095)
Rhyan Sawyer, University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, Stephen A Fuselier, Southwest Research Institute, San Antonio, TX, United States, Joey Mukherjee, Southwest Research Inst, San Antonio, TX, United States, Petrinec M Steven, Lockheed Martin Advanced Technology Center, Palo Alto, CA, United States and Adam Masters, Imperial College London, Department of Physics, London, United Kingdom
The Periodic Flapping and Breathing of Saturn's Magnetodisk During Equinox (220926)
Arianna Milena Sorba, University College London, London, United Kingdom, Nicholas A Achilleos, University College London, Department of Physics and Astronomy, London, United Kingdom, Patrick Guio, The Centre for Planetary Sciences at UCL/Birkbeck, Gower St., London, WC1E 6BT, London, United Kingdom, Christopher Stephen Arridge, Lancaster University, Department of Physics, Lancaster, United Kingdom, Michele Karen Dougherty, Imperial College, London, United Kingdom and Nick Sergis, Academy of Athens, Athens, Greece
Hybrid simulations of radial transport driven by the Rayleigh-Taylor instability (256370)
Blake Hughes Stauffer, University of Alaska Fairbanks, Fairbanks, AK, United States, Peter A Delamere, University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States and Xuanye Ma, Embry-Riddle Aeronautical University, Physical Sciences -- Center for Space and Atmospheric Research, Daytona Beach, FL, United States
New Magnetic Field Model for Saturn From Cassini Radio and Magnetometers Observations: The Birotor Dipole (275009)
Patrick H. M. Galopeau, CNRS, Paris Cedex 16, France
Quasi-periodic latitudinal shift of Saturn’s main auroral emission (269753)
Benjamin Palmaerts1, Elias Roussos2, Denis C Grodent1, Katerina Radioti1, Norbert Krupp3 and Zhonghua Yao4, (1)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (2)Max Planck Institute for Solar System Research, Göttingen, Germany, (3)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (4)Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
Dawnside Variability of Magnetic Field in High Latitude Regions of Saturn's Magnetosphere (256047)
Ewen Henry Davies, Imperial College London, London, SW7, United Kingdom, Adam Masters, Imperial College London, Department of Physics, London, United Kingdom, Michele Karen Dougherty, Imperial College, London, United Kingdom and Nick Sergis, Academy of Athens, Athens, Greece
Distribution and Energization of the Heavy Ions in Saturn’s Magnetosphere (259612)
Tamas I Gombosi, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, Valeriy Tenishev, Univ Michigan, Ann Arbor, United States, Michael R Combi, Univ Michigan, Ann Arbor, MI, United States, Dmitry Borovikov, University of Michigan, Ann Arbor, MI, United States and Leonardo Regoli, JHU Applied Physics Lab, Laurel, United States
The Plasma Proton Environment within Saturn’s inner magnetosphere as Observed by the Cassini Plasma Spectrometer (CAPS) during Saturn Orbit Insertion (290655)
Edward C Sittler Jr, NASA Goddard Space Flight Center, Geospace Physics Laboratory, Greenbelt, United States, Dr. Meredith K Elrod, University of Maryland College Park, Astronomy Department, College Park, United States, Robert E Johnson, University of Virginia, Materials Science and Engineering, Charlottesville, United States, John F Cooper, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Wei-Ling Tseng, Department of Earth Sciences, National Taiwan Normal University, Taipei, Taiwan, H. T. Smith, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Dennis J Chornay, NASA Goddard Space Flight Center, Greenbelt, United States, Mark Shappirio, NASA/GSFC, Greenbelt, MD, United States and David G Simpson, NASA Goddard Space Flight Ctr, Greenbelt, MD, United States
A Large Seasonal Variation of Energetic C+ and CO+ Abundances in Saturn’s Magnetosphere Probably Resulting from Changing Ring Illumination (290835)
Douglas C Hamilton, University of Maryland College Park, College Park, MD, United States and Stephen P Christon, Focused Analysis and Research, Columbia, MD, United States
Analyzing Saturn's Magnetospheric Data After Cassini - Improving and Future-Proofing Cassini / MAPS Tools and Data (252967)
Lawrence E Brown1, Jeremy Faden2, Jon Duane Vandegriff3, William S Kurth4 and Donald G Mitchell1, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Cottage Systems, Iowa City, United States, (3)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (4)University of Iowa, Physics and Astronomy, Iowa City, IA, United States

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