SM44B:
Magnetospheres in the Outer Solar System I

Submit an Abstract to this Session



Session ID#: 32909

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:  George B Hospodarsky, University of Iowa, Physics and Astronomy, Iowa City, IA, 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

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:

Tom Stallard, Northumbria University, Newcastle-Upon-Tyne, United Kingdom, Henrik Melin, University of Leicester, Leicester, LE1, United Kingdom and Rosie Johnson, University of Leicester, Leicester, United Kingdom
Peter A Delamere, University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States, Brandon L Burkholder, University of Alaska Fairbanks, Fairbanks, United States, Xuanye Ma, Embry-Riddle Aeronautical University, Physical Sciences -- Center for Space and Atmospheric Research, Daytona Beach, FL, United States and Katariina Nykyri, NASA Goddard Space Flight Center, Geospace Laboratory, 673, Greenbelt, United States
William S Kurth, University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States and George B Hospodarsky, University of Iowa, Physics and Astronomy, Iowa City, IA, United States
Norbert Krupp1, Elias Roussos2, Donald G Mitchell3, Peter Kollmann3, Chris Paranicas3, Stamatios Mike Krimigis4, Matthew M Hedman5 and Michele Karen Dougherty6, (1)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (2)Max Planck Institute for Solar System Research, Göttingen, Germany, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (4)Academy of Athens, Space, Athens, Greece, (5)University of Idaho, Moscow, United States, (6)Imperial College, London, United Kingdom
Margaret Kivelson, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, CA, United States, Xianzhe Jia, University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States and Caitriona Mary Jackman, University of Southampton, Southampton, United Kingdom
Howard Todd Smith, The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and John D Richardson, MIT, Cambridge, MA, United States
Zachary Christopher Meeks1, Sven Simon2, Slawa Kabanovic1 and Lucas Liuzzo1, (1)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (2)Georgia Institute of Technology, School of Earth and Atmospheric Sciences, Atlanta, United States
Liutauras Rusaitis, University of California Los Angeles, Los Angeles, CA, United States, Krishan K Khurana, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States, Raymond J Walker, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, CA, United States and Margaret Kivelson, UCLA, Los Angeles, United States