SM51E:
Magnetospheres in the Outer Solar System III Posters

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Session ID#: 12489

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 four giant planets (Jupiter, Saturn, Uranus and Neptune) as well as Ganymede’s magnetosphere. The session will accept papers on magnetospheric and auroral processes including magnetosphere-ionosphere coupling, plasma transport, tail dynamics, rotational modulations, boundaries, and the role of the solar wind. 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, such as Cassini, Juno, and JUICE.
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 George B Hospodarsky, University of Iowa, Iowa City, IA, 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

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

2704 Auroral phenomena [MAGNETOSPHERIC PHYSICS]
2731 Magnetosphere: outer [MAGNETOSPHERIC PHYSICS]
2756 Planetary magnetospheres [MAGNETOSPHERIC PHYSICS]
6222 Ganymede [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Abstracts Submitted to this Session:

Interactions Between Energetic Electrons and Realistic Whistler Mode Waves in the Jovian Magnetosphere (125061)
Maria de Soria-Santacruz Pich1, Alexander Drozdov2, John Douglas Menietti3, Henry Berry Garrett4, Adam C Kellerman5 and Yuri Y. Shprits2,6, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)University of California Los Angeles, EPSS, Los Angeles, CA, United States, (3)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (4)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (5)University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States, (6)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany
Trading Places: Can Interchange Energy Solve the Torus Energy Crisis? (142791)
Katherine M Ramer, University of California Los Angeles, Los Angeles, CA, United States, Margaret Kivelson, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, CA, United States and Krishan K Khurana, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States
Radial transport from the Io plasma torus: driven from the inside out or outside in? (147535)
Jeffrey P Morgenthaler, Planetary Science Institute Fort Kent, Fort Kent, United States, Max Marconi, Organization Not Listed, Washington, DC, United States, Ronald J Oliversen, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Roland Carey Woodward Jr, University of Wisconsin Eau Claire, Eau Claire, WI, United States
Asymmetries in Jupiter's Magnetosphere (147859)
Emmanuel Chané, Katholieke Universiteit Leuven, Leuven, Belgium
Heavy Plasma Ions in the Jovian Magnetosphere: What will Juno Encounter? (160309)
Logan Dougherty1, Fran Bagenal2 and Kaleb Michael Bodisch1, (1)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (2)University of Colorado at Boulder, Boulder, CO, United States
Protons in Jupiter’s Magnetosphere (160493)
Kaleb Michael Bodisch1, Fran Bagenal2 and Logan Dougherty1, (1)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (2)University of Colorado at Boulder, Boulder, CO, United States
Method to observe O+ and S2+ by the JADE-I instrument on NASA’s Juno mission to Jupiter (171586)
Thomas K Kim1,2, Philip W Valek2, David J McComas3, Scott J Bolton4, Frederic Allegrini4, Nigel G Angold5, Fran Bagenal6, Kyung Chae2, John E P Connerney7, Robert W Ebert2, Steven Levin8, Chad E Loeffler2, Philippe Louarn9, Craig J Pollock10, Drake A Ranquist11, Michelle L Reno2, Jamey Szalay2, Michelle F Thomsen12, Scott Weidner13, Robert J Wilson14 and Jenna Lynn Zink1, (1)University of Texas at San Antonio, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)Princeton University, Department of Astrophysical Sciences and Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (4)Southwest Research Institute, San Antonio, United States, (5)Angold Consulting for SwRI, La Cañada, CA, United States, (6)University of Colorado at Boulder, Boulder, CO, United States, (7)Space Research Corporation, Annapolis, United States, (8)Jet Propulsion Laboratory, Pasadena, CA, United States, (9)IRAP, Toulouse, France, (10)University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States, (11)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (12)Planetary Science Institute Tucson, Tucson, AZ, United States, (13)Princeton University, Princeton, NJ, United States, (14)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
MHD Modeling of Jupiter’s Magnetosphere using the Space Weather Modeling Framework (SWMF): Preliminary Results (153548)
Yash Sarkango, University of Minnesota, School of Physics and Astronomy, Minneapolis, United States, Xianzhe Jia, University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, Gabor Toth, University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States and Kenneth C Hansen, University of Michigan Ann Arbor, Ann Arbor, MI, United States
Interaction of a Variable Solar Wind with Jupiter’s Magnetosphere: A 3D MHD Simulation (177552)
Drake A Ranquist, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, Fran Bagenal, University of Colorado at Boulder, Boulder, CO, United States, Peter A Delamere, University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States and Xuanye Ma, University of Alaska Fairbanks, Fairbanks, United States
Jupiter’s Io-D Decametric Source Morphology using the Long Wavelength Array Station 1 (180833)
Charles A Higgins, Middle Tennessee State University, Physics and Astronomy, Murfreesboro, TN, United States, Tracy Clarke, Naval Research Lab DC, 7200, Washington, DC, United States, Kazumasa Imai, Kochi Natl College Tech, Nankoku City Kochi, Japan, Masafumi Imai, University of Iowa, Physics and Astronomy, Iowa City, IA, United States, Francisco J Reyes, University of Florida, Astronomy, Ft Walton Beach, FL, United States and James Thieman, NASA/GSFC, Greenbelt, MD, United States
Model Predictions and Ground-based Observations for Jupiter's Magnetospheric Environment: Application to the JUICE and Juno Missions (172996)
Nicholas A Achilleos1, Patrick Guio1, Christopher Stephen Arridge2, Licia C Ray3, Japheth N Yates4, Stephen Fossey1, Giorgio Savini1, Mick Pearson1, Nathalie Fernando1, Roman Gerasimov1 and Tom Murat1, (1)University College London, Centre for Planetary Sciences (at UCL/Birkbeck), London, United Kingdom, (2)Lancaster University, Department of Physics, Lancaster, United Kingdom, (3)Mullard Space Science Laboratory, Dorking, United Kingdom, (4)Imperial College London, London, United Kingdom
Charged Particle Dynamics in a Magnetodisc-Field Structure (175052)
Patrick Guio1, Will O'Brien1, Nicholas A Achilleos1 and Christopher Stephen Arridge2, (1)University College London, Centre for Planetary Sciences (at UCL/Birkbeck), London, United Kingdom, (2)Lancaster University, Physics Department, Lancaster, United Kingdom
On the stability of fast rotating magentodiscs (194467)
Bishwa Raj Neupane1, Peter A Delamere2 and Xuanye Ma1, (1)University of Alaska Fairbanks, Fairbanks, United States, (2)University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States
Radiation Science Enabled by the Radiation Monitoring Subsystem (RMS) for the Planned Europa Mission (181667)
Insoo Jun1, Chris Paranicas2, John O Goldsten3, Richard Meitzler4, Patrick N Peplowski2 and Richard Maurer2, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (3)Johns Hopkins Univ/APL, Laurel, MD, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, United States
A Comprehensive Analysis of Ion Cyclotron Waves in the Equatorial Magnetosphere of Saturn (128423)
Zachary Christopher Meeks, Georgia Institute of Technology Main Campus, Atlanta, GA, United States and Sven Simon, Georgia Institute of Technology Main Campus, Atlanta, United States
26-day Periodicities in Low-Energy Electrons at Saturn (126373)
James F Carbary, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
On the origin of the 1-hour pulsations in the Saturn's magnetosphere (167445)
Liutauras Rusaitis1, Raymond J Walker2, Krishan K Khurana3 and Margaret Kivelson2, (1)University of California Los Angeles, Los Angeles, CA, United States, (2)University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, CA, United States, (3)University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States
An Isolated, Bright Cusp Aurora Associated with Dayside Reconnection at Saturn (147010)
Joe Kinrade1, Sarah Victoria Badman2, Christopher Stephen Arridge3, Chihiro Tao4, Gabrielle Provan5, Michele Karen Dougherty6 and Adrian Grocott1, (1)Lancaster University, Physics Department, Lancaster, United Kingdom, (2)University of Lancaster, Lancaster, United Kingdom, (3)University College London, Mullard Space Science Laboratory, London, United Kingdom, (4)IRAP, Toulouse, France, (5)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (6)Imperial College London, London, United Kingdom
Low Frequency Extensions of the Saturn Kilometric Radiation as a Proxy for Magnetospheric Dynamics. (171693)
Joe Reed1, Caitriona Mary Jackman2, Daniel K Whiter2, William S Kurth3 and Laurent Lamy4, (1)University of Southampton, Southampton, SO14, United Kingdom, (2)University of Southampton, Southampton, United Kingdom, (3)University of Iowa, Iowa City, IA, United States, (4)Paris Observatory Meudon, LIRA, Meudon, France
Energy Dissipation in Saturn’s Magnetotail: A Comparative Magnetotail Approach (144655)
Zhonghua Yao1, Andrew J Coates2, Licia C Ray3, Jonathan Rae1, Denis C Grodent4, Katerina Radioti4, William Dunn5, Geraint Jones6 and Jack H Waite7, (1)University College London, London, United Kingdom, (2)University College London, Centre for Planetary Sciences (at UCL/Birkbeck), London, United Kingdom, (3)Mullard Space Science Laboratory, Dorking, United Kingdom, (4)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (5)University College London, Department of Phyics and Astronomy, London, United Kingdom, (6)University College London, Mullard Space Science Laboratory, London, United Kingdom, (7)Southwest Research Institute, San Antonio, TX, United States
Galactic Cosmic Rays access to the upper atmosphere and rings of Saturn (135122)
Anna Kotova1,2, Elias Roussos3, Norbert Krupp3 and Iannis S Dandouras4, (1)University Paul Sabatier Toulouse III, Toulouse Cedex 09, France, (2)Max Planck Institute for Solar System Research, Gottingen, Germany, (3)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (4)IRAP, Toulouse, France
Modelling Photoelectron Production in the Enceladus Plume and Comparison with Observations by CAPS-ELS (133383)
Sam A Taylor1, Andrew J Coates1, Geraint Jones1, Anne Wellbrock1 and Jack H Waite2, (1)University College London, Mullard Space Science Laboratory, London, United Kingdom, (2)Southwest Research Institute, San Antonio, TX, United States
An Updated Model of Saturn's Internal Magnetic Field (151458)
Marcia E Burton, NASA Jet Propulsion Laboratory, Pasadena, CA, United States and Michele Karen Dougherty, Imperial College London, London, United Kingdom
Magnetic Flux Circulation in the Saturnian Magnetosphere Revisited (129533)
Hairong Lai, Sun Yat-Sen University, Guangzhou, China, Christopher T Russell, University of California, IGPP/EPSS, Los Angeles, CA, United States, Ying-Dong Jia, University of California Los Angeles, Los Angeles, CA, United States, Adam Masters, Imperial College London, Department of Physics, London, United Kingdom and Michele Karen Dougherty, Imperial College London, London, United Kingdom
Dissecting Saturn’s magnetosphere using ion pitch angle distributions (158938)
David Andrew Laubner1, George B Clark2, Jon Duane Vandegriff1, Chris Paranicas1, Peter Kollmann1, Donald G Mitchell1 and Howard Todd Smith3, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (3)The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Detecting dust hits at Enceladus, Saturn and beyond using CAPS / ELS data from Cassini (161072)
Payton James Stoneberger1, Geraint Jones2, Jack H Waite3 and Jon Duane Vandegriff1, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)University College London, Mullard Space Science Laboratory, London, United Kingdom, (3)Southwest Research Institute, San Antonio, TX, United States
Investigating the Evolution and Fate of Injection Events at Saturn Using Cassini Data (164027)
Abigail Azari1, Michael Warren Liemohn2, Xianzhe Jia3, Donald G Mitchell4, Abigail M Rymer5 and Jon Duane Vandegriff4, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (2)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, United States
Does Magnetosphere-Ionosphere Coupling, and the Associated Energetic Field Aligned Electron Beams Created Outside 12 RS, Populate Saturn’s Radiation Belts? (164404)
Abigail M Rymer1, Barry Mauk2, James F Carbary2, Peter Kollmann2, George B Clark3, Donald G Mitchell2 and Andrew J Coates4, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (3)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)University College London, Centre for Planetary Sciences (at UCL/Birkbeck), London, United Kingdom
iPhone App for Cassini's Magnetospheric Imaging Instrument (MIMI) Browse Products (176416)
Helene Young Myers1, Martha Bolz Kusterer1, Donald G Mitchell1, Robert J Steele2 and Jon Duane Vandegriff1, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Johns Hopkins University, Laurel, MD, United States
Suprathermal H2+ Ions in the Solar Wind, Magnetosheath, and Magnetosphere near Titan (190730)
Douglas C Hamilton1, M.a. Khaial1, Cesar Bertucci2 and Donald G Mitchell3, (1)University of Maryland College Park, College Park, MD, United States, (2)Consejo Nacional de Investigaciones Científicas y Técnicas, Buenos Aires, Argentina, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Turbulent Magnetic Fields Near Saturn's Magnetopause Boundary (183650)
Brandon L Burkholder1, Xuanye Ma1, Vitaliy Matveevich Kaminker2 and Peter A Delamere3, (1)University of Alaska Fairbanks, Fairbanks, United States, (2)University of Alaska Fairbanks, Fairbanks, AK, United States, (3)University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States
Understanding the Pluto-Charon Plasma Environment during the New Horizons Encounter (132634)
John M Hale, Georgia Institute of Technology Main Campus, Atlanta, GA, United States and Carol S Paty, University of Oregon, Earth Sciences, Eugene, OR, United States
Multi-fluid MHD study of the solar wind interaction with Pluto (199579)
Chuanfei Dong1, Yingjuan Ma2, David J McComas3,4, Amitava Bhattacharjee5, Eric Zirnstein4, Gabor Toth6, Janet G Luhmann7 and Liang Wang8, (1)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (2)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, United States, (3)Princeton University, Department of Astrophysical Sciences and Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (4)Southwest Research Institute, San Antonio, TX, United States, (5)Princeton University, Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (6)University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (7)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (8)Princeton University, Princeton, NJ, United States

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