P31C:
Juno's Exploration of Jupiter and the Earth-Based Collaborative Campaign III Posters

Submit an Abstract to this Session



Session ID#: 21884

Session Description:
NASA's Juno mission to Jupiter launched in 2011 and arrived at Jupiter on July 4, 2016. Juno's scientific objectives include the study of Jupiter's interior, atmosphere and magnetosphere with the goal of understanding Jupiter's origin, formation and evolution. An extensive campaign of Earth based observations of Jupiter and the solar wind were orchestrated to complement Juno measurements during Juno's approach to Jupiter and during its orbital mission around Jupiter. This session provides results from the Juno measurements and the collaborative campaign (including Hisaki) during the first year of Juno's prime mission. Scientific results include Jupiter's interior structure, magnetic field, deep atmospheric dynamics and composition, and the first in-situ exploration of Jupiter's polar magnetosphere and aurorae.
Primary Convener:  Scott J Bolton, Southwest Research Institute, San Antonio, United States
Conveners:  Fran Bagenal, University of Colorado at Boulder, Boulder, CO, United States, Steven Levin, Jet Propulsion Laboratory, Pasadena, CA, United States and John E P Connerney, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Chairs:  Philip W Valek, Southwest Research Institute, San Antonio, United States and Chris Paranicas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
OSPA Liaison:  Glenn S Orton, Jet Propulsion Laboratory, Pasadena, CA, United States
Co-Organized with:
Planetary Sciences, Atmospheric Sciences, SPA-Solar and Heliospheric Physics, and SPA-Magnetospheric Physics
Index Terms:

2756 Planetary magnetospheres [MAGNETOSPHERIC PHYSICS]
5704 Atmospheres [PLANETARY SCIENCES: FLUID PLANETS]
5724 Interiors [PLANETARY SCIENCES: FLUID PLANETS]
6220 Jupiter [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Abstracts Submitted to this Session:

Low- and high-order gravitational harmonics of interior models for rigidly rotating Jupiter (224034)
Nadine Nettelmann, University of Rostock, Rostock, Germany
Investigating Jupiter's Deep Flow Structure using the Juno Magnetic and Gravity Measurements (238128)
Keren Duer1, Eli Galanti2, Hao Cao3 and Yohai Kaspi2, (1)Weizmann Institute of Science, Rehovot, Israel, (2)Weizmann Institute of Science, Earth and Planetary Sciences, Rehovot, Israel, (3)California Institute of Technology, Pasadena, United States
Ammonia in Jupiter’s troposphere: a comparison of ground-based 5-μm high-resolution spectroscopy and Juno MWR observations (262714)
Rohini Giles, Jet Propulsion Laboratory/ California Institute of Technology, Pasadena, United States, Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, Leigh N. Fletcher, University of Leicester, Leicester, United Kingdom, Patrick GJ Irwin, University of Oxford, Atmospheric, Oceanic, and Planetary Physics laboratory, Oxford, United Kingdom and James Andrew Sinclair, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, CA, United States
The Jovian rings as observed from Jupiter. (269500)
Anastassia Malinnikova Bang1, John Leif Joergensen2, Peter S Joergensen2, Troelz Denver3, John E P Connerney4, Scott J Bolton5 and Steven Levin6, (1)Technical University of Denmark, Kgs. Lyngby, Denmark, (2)DTU Space, National Space Institute, Technical University of Denmark, Kgs Lyngby, Denmark, (3)Technical University of Denmark, DTU Space, Kgs. Lyngby, Denmark, (4)Space Research Corporation, Annapolis, United States, (5)Southwest Research Institute, San Antonio, United States, (6)Jet Propulsion Laboratory, Pasadena, United States
Water and Ammonia Abundances in Jupiter’s South Equatorial Belt and Equatorial Zone at the time of Juno Perijoves 4 to 6 (285499)
Gordon L Bjoraker, NASA Goddard Space Flight Center, Greenbelt, United States, Imke De Pater, University of California Berkeley, Departments of Astronomy and of Earth and Planetary Science, Berkeley, United States, Michael H. Wong, U. Berkeley, Berkeley, United States, Mate Adamkovics, Clemson University, Department of Physics and Astronomy, Clemson, United States, Tilak Hewagama, University of Maryland, College Park, Astronomy, College Park, MD, United States and Glenn Orton, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States
Latitudinal Variation of Germane in Jovian Atmosphere (295834)
Ali Hyder, Hofstra University, Hempstead, NY, United States, Jonathan I Lunine, Cornell University, Department of Astronomy, Ithaca, NY, United States and Dong Wang, Cornell University, Ithaca, NY, United States
Jupiter’s Dawn Magnetosheath and Magnetopause as Measured by Juno (278391)
Drake A Ranquist, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, Fran Bagenal, University of Colorado at Boulder, Boulder, CO, United States, George B Hospodarsky, Univ. of Iowa, Iowa City, IA, United States, Robert J Wilson, LASP, Boulder, United States, Philip W Valek, Southwest Research Institute, San Antonio, United States, John E P Connerney, Space Research Corporation, Annapolis, United States, William S Kurth, University of Iowa, Iowa City, IA, United States, Barry Mauk, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Daniel J Gershman, NASA Goddard Space Flight Center, Greenbelt, United States
Juno Perijove 1 radio occultation of the Io plasma torus (279802)
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, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and Parker C Hinton, Department of Astrophysical and Planetary Sciences, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
The Jovian Magnetodisc Mapped at High Latitude by the Juno Spacecraft (285019)
Lori Spalsbury, ADNET Systems Inc. Greenbelt, Greenbelt, MD, United States, Marissa F. Vogt, Boston University, Boston, United States and John E P Connerney, Space Research Corporation, Annapolis, United States
Evidence of field-aligned currents in Jupiter's polar magnetosphere (286249)
Stavros Kotsiaros, NASA Goddard Space Flight Center, Greenbelt, MD, United States, John E P Connerney, Space Research Corporation, Annapolis, United States, Barry Mauk, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, George B Clark, Applied Physics Laboratory Johns Hopkins, Laurel, United States, Scott J Bolton, Southwest Research Institute, San Antonio, United States and Steven Levin, Jet Propulsion Laboratory, Pasadena, CA, United States
Cold blobs of protons in Jupiter's outer magnetosphere as observed by Juno's JADE (289271)
Robert J Wilson1, Fran Bagenal2, Philip W Valek3, Frederic Allegrini4, Nigel G Angold5, Kyung Chae6, Robert W Ebert7, Thomas K Kim6, Chad Loeffler8, Philippe Louarn9, David J McComas10, Craig J Pollock11, Drake A Ranquist12, Chelle Reno13, Jamey R Szalay14, Michelle F Thomsen15, Scot Weidner13, Scott J Bolton3 and Steven Levin16, (1)LASP, Boulder, United States, (2)University of Colorado at Boulder, Boulder, CO, United States, (3)Southwest Research Institute, San Antonio, United States, (4)Southwest Research Inst, San Antonio, United States, (5)Angold Consulting for SwRI, La Cañada, CA, United States, (6)Southwest Research Institute, San Antonio, TX, United States, (7)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (8)Southwest Research Inst, San Antonio, TX, United States, (9)IRAP, Toulouse, France, (10)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (11)Denali Scientific, San Antonio, TX, United States, (12)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (13)Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (14)Princeton University, Department of Astrophysical Sciences, Princeton, United States, (15)Los Alamos National Laboratory, Los Alamos, NM, United States, (16)Jet Propulsion Laboratory, Pasadena, United States
Chandra observations of Jupiter’s X-ray Aurora during Juno upstream and apojove intervals (289595)
Caitriona Mary Jackman1, William Dunn2, Ralph Kraft3, Randy Gladstone4, Graziella Branduardi-Raymont5, Christian Knigge1, Diego Altamirano1, Ronald Elsner6 and Joshua Kammer7, (1)University of Southampton, Southampton, United Kingdom, (2)University College London, Department of Phyics and Astronomy, London, United Kingdom, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)Southwest Research Institute, San Antonio, United States, (5)University College London, Mullard Space Science Laboratory, London, United Kingdom, (6)NASA Marshall Space Flight Center, Huntsville, AL, United States, (7)Southwest Research Institute, Boulder, CO, United States
Jovian Space Weather in the Juno Era: Remote Observations (290261)
Robert J. MacDowall1, Michael J Reiner2, William M Farrell1 and John E P Connerney3, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Catholic Univ & GSFC, Greenbelt, MD, United States, (3)Space Research Corporation, Annapolis, United States
Systematic capture of MeV electron beams by MWR (274490)
Daniel Santos-Costa1, Amadeo Bellotti2, Mike Janssen3, Samuel Gulkis4, Andrew P. Ingersoll4, Steven Levin5, Paul G Steffes2, Shannon Thomas Brown6, Virgil Adumitroaie6, Fabiano A Oyafuso5, George B Clark7, Barry Mauk8, Heidi N Becker9, John Leif Joergensen10, Alberto Adriani11, John E P Connerney12, Randy Gladstone13, Vincent Hue1, Denis C Grodent14, Bertrand Bonfond14, Robert W Ebert15, Philip W Valek13, Scott J Bolton13 and Richard M Thorne16, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (3)Jet Propulsion Laboratory, Pasadena, CA, United States, (4)California Institute of Technology, Pasadena, CA, United States, (5)Jet Propulsion Laboratory, Pasadena, United States, (6)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (7)Applied Physics Laboratory Johns Hopkins, Laurel, United States, (8)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (9)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (10)Technical University of Denmark, DTU Space, Kgs. Lyngby, Denmark, (11)IAPS-INAF, Rome, Italy, (12)Space Research Corporation, Annapolis, United States, (13)Southwest Research Institute, San Antonio, United States, (14)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (15)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (16)UCLA, Los Angeles, CA, United States
Juno/JEDI observations of energetic particles in Jupiter’s polar magnetosphere (276244)
Dennis K Haggerty1, Barry Mauk1, Chris Paranicas1, George B Clark2, Peter Kollmann3, Abigail M Rymer1, Scott J Bolton4, John E P Connerney5, Steven Levin6 and Thomas Cravens7, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Applied Physics Laboratory Johns Hopkins, Laurel, United States, (3)The Applied Physics Laboratory, John Hopkins University, Laurel, United States, (4)Southwest Research Institute, San Antonio, United States, (5)Space Research Corporation, Annapolis, United States, (6)Jet Propulsion Laboratory, Pasadena, United States, (7)University of Kansas, Physics and Astronomy, Lawrence, United States
A global model of magnetic reconnection and growth of the Kelvin-Helmholtz instability at Jupiter’s magnetopause (210631)
Adam Masters, Imperial College London, Department of Physics, London, United Kingdom
Probing Jupiter’s Radiation Environment with Juno-UVS (213446)
Joshua Kammer1, Randy Gladstone2, Thomas K Greathouse2, Vincent Hue1, Maarten H Versteeg2, Michael Wayne Davis1, Daniel Santos-Costa1, Heidi N Becker3, Scott J Bolton2, John E P Connerney4 and Steven Levin5, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (4)Space Research Corporation, Annapolis, United States, (5)Jet Propulsion Laboratory, Pasadena, United States
Electron Pitch Angle Distributions Along Field Lines Connected to the Auroral Region from ~25 to ~1.2 RJ Measured by the Jovian Auroral Distributions Experiment-Electrons (JADE-E) on Juno (232359)
Frederic Allegrini1, Fran Bagenal2, Scott J Bolton3, Bertrand Bonfond4, Kyung Chae1, George B Clark5, John E P Connerney6, Robert W Ebert7, Randy Gladstone3, Vincent Hue1, George B Hospodarsky8, Thomas K Kim1, William S Kurth9, Steven Levin10, Philippe Louarn11, Barry Mauk12, David J McComas13, Craig J Pollock14, Drake A Ranquist15, Michelle L Reno16, Joachim Saur17, Jamey Szalay1, Michelle F Thomsen18, Philip W Valek3 and Robert J Wilson19, (1)Southwest Research Institute, San Antonio, TX, United States, (2)University of Colorado at Boulder, Boulder, CO, United States, (3)Southwest Research Institute, San Antonio, United States, (4)Université de Liège, Space sciences, Technologies & Astrophysics Research Institute, Liege, Belgium, (5)Applied Physics Laboratory Johns Hopkins, Laurel, United States, (6)Space Research Corporation, Annapolis, United States, (7)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (8)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (9)Univ. of Iowa, Iowa City, IA, United States, (10)Jet Propulsion Laboratory, Pasadena, CA, United States, (11)IRAP, Toulouse, France, (12)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (13)Princeton University, Department of Astrophysical Sciences and Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (14)Denali Scientific, Healy, AK, United States, (15)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (16)Austin Mission Consulting, Austin, TX, United States, (17)University of Cologne, Cologne, Germany, (18)Los Alamos National Laboratory, Los Alamos, NM, United States, (19)Univ Colorado, Boulder, United States
Studying and Understanding the Jovian Aurora Based on Measurements from the Juno MWR Taken during Perijove 5 (240440)
Amadeo Bellotti1, Paul G Steffes1 and Michael A Janssen2, (1)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States
Characterizing the Io Plasma Torus with Juno radio science experiment (240857)
Marco Zannoni, University of Bologna, Department of Industrial Engineering, Forlì, Italy, Daniele Durante, Sapienza University of Rome, Rome, Italy, Luciano Iess, Jet Propulsion Laboratory, Pasadena, CA, United States and Paolo Tortora, University of Bologna, Centro Interdipartimentale di Ricerca Industriale Aerospaziale, Forlì, Italy
Observations by Juno’s Radiation Monitoring Investigation During the First Year at Jupiter (246185)
Heidi N Becker1, Virgil Adumitroaie2, James W Alexander3, Ingrid Daubar3, John Leif Joergensen4, Troelz Denver5, Mathias Benn5, Alberto Adriani6, Alessandro Mura6, Andrea Cicchetti6, Raffaella Noschese7, John E P Connerney8, Randy Gladstone9, Vincent Hue10, Maarten Versteeg10, Daniel Santos-Costa10, Scott J Bolton9, Steven Levin1 and Richard M Thorne11, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (4)DTU Space, National Space Institute, Technical University of Denmark, Kgs Lyngby, Denmark, (5)Technical University of Denmark, DTU Space, Kgs. Lyngby, Denmark, (6)IAPS-INAF, Rome, Italy, (7)INAF-IAPS, Rome, Italy, (8)Space Research Corporation, Annapolis, United States, (9)Southwest Research Institute, San Antonio, United States, (10)Southwest Research Institute, San Antonio, TX, United States, (11)University of California Los Angeles, Los Angeles, CA, United States
Jupiter’s X-ray Auroral Pulsations and Spectra During Juno Perijove 7 (261755)
William Dunn1, Graziella Branduardi-Raymont2, Licia C Ray3, Caitriona Mary Jackman4, Ralph Kraft5, Randy Gladstone6, Zhonghua Yao7, Jonathan Rae2, Rebecca Gray8, Ronald Elsner9, Denis C Grodent10, Jonathan D Nichols11, Peter G Ford12, Jan Uwe Ness13, Joshua Kammer14 and Pedro Rodriguez13, (1)University College London, Department of Phyics and Astronomy, London, United Kingdom, (2)University College London, Mullard Space Science Laboratory, London, United Kingdom, (3)Mullard Space Science Laboratory, Dorking, United Kingdom, (4)University of Southampton, Southampton, United Kingdom, (5)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (6)Southwest Research Institute, San Antonio, United States, (7)Chinese Academy of Sciences, Beijing, China, (8)University of Lancaster, Lancaster, United Kingdom, (9)NASA Marshall Space Flight Center, Huntsville, AL, United States, (10)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (11)University of Leicester, School of Physics and Astronomy, Leicester, LE1, United Kingdom, (12)MIT, Cambridge, MA, United States, (13)European Space Agency, Villanueva De La Can, Spain, (14)Southwest Research Institute, Boulder, CO, United States
Juno-UVS observation of the Io footprint: Influence of Io’s local environment and passage into eclipse on the strength of the interaction (266533)
Vincent Hue1, Randy Gladstone2, Thomas K Greathouse2, Maarten Versteeg1, Bertrand Bonfond3, Joachim Saur4, Michael W Davis2, Lorenz Roth5, Denis C Grodent3, Jean-Claude M. C. Gerard3, Joshua Kammer6, Scott J Bolton2, Steven Levin7 and John E P Connerney8, (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)University of Cologne, Cologne, Germany, (5)KTH Royal Institute of Technology, Division of Space and Plasma Physics, School of Electrical Engineering, Stockholm, Sweden, (6)Southwest Research Institute, Boulder, CO, United States, (7)Jet Propulsion Laboratory, Pasadena, United States, (8)Space Research Corporation, Annapolis, United States
Dynamical and Chemical Tracers in Jupiter’s Troposphere and Stratosphere from the Earth-Based Infrared Juno Support Campaign (270766)
Henrik Melin1, Leigh N. Fletcher2, Padraig T Donnelly2, Thomas Greathouse3, John Lacy4, Glenn Orton5, Rohini Giles6, James Andrew Sinclair7 and Patrick GJ Irwin8, (1)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (2)University of Leicester, Leicester, United Kingdom, (3)Southwest Research Inst, San Antonio, United States, (4)University of Texas at Austin, Austin, TX, United States, (5)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (6)California Institute of Technology, Pasadena, CA, United States, (7)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, CA, United States, (8)University of Oxford, Atmospheric, Oceanic, and Planetary Physics laboratory, Oxford, United Kingdom
The absent magnetospheric cushion near Jupiter’s dawn terminator? (271851)
Daniel J Gershman, University of Maryland College Park, College Park, United States, Gina A DiBraccio, NASA Goddard Space Flight Center, Greenbelt, MD, United States, John E P Connerney, Space Research Corporation, Annapolis, United States, Fran Bagenal, University of Colorado at Boulder, Boulder, CO, United States, George B Clark, Applied Physics Laboratory Johns Hopkins, Laurel, United States, Barry Mauk, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, George B Hospodarsky, Univ. of Iowa, Iowa City, IA, United States, William S Kurth, University of Iowa, Iowa City, IA, United States, Steven Levin, Jet Propulsion Laboratory, Pasadena, United States and Scott J Bolton, Southwest Research Institute, San Antonio, United States
Spatial and Temporal Variability of Southern Auroral Emissions in the IR from JIRAM/Juno Data (272019)
Francesca Altieri1, Maria Luisa Moriconi2, Alessandro Mura1, Alberto Adriani1, Davide Grassi1, Alessandra Migliorini1, Jean-Claude M. C. Gerard3, Bianca Maria Dinelli2, Federico Fabiano4, Gianrico Filacchione1, Giuseppe Sindoni1, Federico Tosi5, Giuseppe Piccioni1, Raffaella Noschese5, Andrea Cicchetti1, Roberto Sordini5, Scott J Bolton6, John E P Connerney7, Sushil K Atreya8, Steven Levin9, Jonathan I Lunine10, Diego Turrini1, Stefania Stefani1, Angelo Olivieri11 and Christina Plainaki12, (1)IAPS-INAF, Rome, Italy, (2)CNR Institute of Atmospheric Sciences and Climate, Bologna, Italy, (3)Université de Liège, Liège, Belgium, (4)CNR, Institute of Atmospheric Sciences and Climate, Bologna, Italy, (5)INAF-IAPS, Rome, Italy, (6)Southwest Research Institute, San Antonio, United States, (7)Space Research Corporation, Annapolis, United States, (8)University of Michigan, Ann Arbor, United States, (9)Jet Propulsion Laboratory, Pasadena, CA, United States, (10)Cornell University, Department of Astronomy, Ithaca, NY, United States, (11)Italian Space Agency, Rome, Italy, (12)ASI, Rome, Italy
Juno observations in the sources of hectometric radiation: role of electron conics (228148)
Philippe Louarn1, Frederic Allegrini2, Philip W Valek3, David J McComas4, William S Kurth5, Nicolas André6, Fran Bagenal7, Scott J Bolton3, John E P Connerney8, Robert W Ebert9, Masafumi Imai10, Steven Levin11, Jamey Szalay12, Scott Weidner13 and Robert J Wilson14, (1)IRAP, Toulouse, France, (2)Southwest Research Inst, San Antonio, United States, (3)Southwest Research Institute, San Antonio, United States, (4)Princeton University, Department of Astrophysical Sciences and Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (5)University of Iowa, Iowa City, IA, United States, (6)IRAP, CNRS, Toulouse, France, (7)University of Colorado at Boulder, Boulder, CO, United States, (8)Space Research Corporation, Annapolis, United States, (9)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (10)Kyoto University, Kyoto, Japan, (11)Jet Propulsion Laboratory, Pasadena, United States, (12)Southwest Research Institute, San Antonio, TX, United States, (13)Princeton University, Princeton, NJ, United States, (14)LASP, Boulder, United States
Plasma sheet properties observed by Juno at Jupiter (285868)
Fran Bagenal1, Robert J Wilson2, Philip W Valek3, Frederic Allegrini4, Nigel G Angold5, Kyung Chae6, Robert W Ebert7, Thomas K Kim6, Philippe Louarn8, Chad E Loeffler6, David J McComas9, Drake A Ranquist10, Chelle Reno11, Jamey R Szalay12, Michelle F Thomsen13, Scot Weidner11, Scott J Bolton3, John E P Connerney14, Steven Levin15, Barry Mauk16 and William S Kurth17, (1)University of Colorado at Boulder, Boulder, CO, United States, (2)LASP, Boulder, United States, (3)Southwest Research Institute, San Antonio, United States, (4)Southwest Research Inst, San Antonio, United States, (5)Angold Consulting for SwRI, La Cañada, CA, United States, (6)Southwest Research Institute, San Antonio, TX, United States, (7)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (8)IRAP, Toulouse, France, (9)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (10)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (11)Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (12)Princeton University, Department of Astrophysical Sciences, Princeton, United States, (13)Los Alamos National Laboratory, Los Alamos, NM, United States, (14)Space Research Corporation, Annapolis, United States, (15)Jet Propulsion Laboratory, Pasadena, CA, United States, (16)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (17)University of Iowa, Iowa City, IA, United States
Wave Particle Interactions in Jupiter's Magnetosphere and Related Stochastic Auroral Particle Acceleration by Kinetic Alfvén Waves (229043)
Joachim Saur, University of Cologne, Institute of Geophysics and Meteorology, Cologne, Germany, Anne Schreiner, Organization Not Listed, Washington, DC, United States, Barry Mauk, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, George B Clark, Applied Physics Laboratory Johns Hopkins, Laurel, United States, Peter Kollmann, The Applied Physics Laboratory, John Hopkins University, Laurel, United States, Robert W Ebert, University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States and Frederic Allegrini, Southwest Research Inst, San Antonio, United States
GCM studies on Jovian polar dynamics (261699)
Fachreddin Tabataba-Vakili1, Glenn Orton2, Cheng Li3, Roland MB Young4, Peter L Read5 and Andrew P. Ingersoll3, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (3)California Institute of Technology, Pasadena, CA, United States, (4)University of Oxford, Oxford, United Kingdom, (5)University of Oxford, AOPP, Oxford, United Kingdom

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