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      Diverse Electron and Ion Acceleration Characteristics Observed Over Jupiter's Main Aurora

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          Most cited references24

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          New models of Jupiter's magnetic field constrained by the Io flux tube footprint

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            Jupiter's interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft.

            On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing less than 5000 kilometers above the equatorial cloud tops. Images of Jupiter's poles show a chaotic scene, unlike Saturn's poles. Microwave sounding reveals weather features at pressures deeper than 100 bars, dominated by an ammonia-rich, narrow low-latitude plume resembling a deeper, wider version of Earth's Hadley cell. Near-infrared mapping reveals the relative humidity within prominent downwelling regions. Juno's measured gravity field differs substantially from the last available estimate and is one order of magnitude more precise. This has implications for the distribution of heavy elements in the interior, including the existence and mass of Jupiter's core. The observed magnetic field exhibits smaller spatial variations than expected, indicative of a rich harmonic content.
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              The Juno Magnetic Field Investigation

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                Author and article information

                Journal
                Geophysical Research Letters
                Geophys. Res. Lett.
                Wiley
                0094-8276
                1944-8007
                February 12 2018
                February 16 2018
                February 15 2018
                February 16 2018
                : 45
                : 3
                : 1277-1285
                Affiliations
                [1 ]Applied Physics LaboratoryThe Johns Hopkins University Laurel MD USA
                [2 ]Southwest Research Institute San Antonio TX USA
                [3 ]Jet Propulsion Laboratory Pasadena CA USA
                [4 ]Instituo di Astofisica e Planetologia SpazialiInstituto Nazionale di Astrofisica Rome Italy
                [5 ]Physics and Astronomy DepartmentUniversity of Texas at San Antonio San Antonio TX USA
                [6 ]Laboratory for Atmospheric and Space PhysicsUniversity of Colorado Boulder Boulder CO USA
                [7 ]LPAP, Space Sciences, Technologies and Astrophysics Research InstituteUniversité de Liège Liège Belgium
                [8 ]NASA Goddard Space Flight Center Greenbelt MD USA
                [9 ]Department of Physics and AstronomyUniversity of Iowa Iowa City IA USA
                [10 ]Department of Astrophysical SciencesPrinceton University Princeton NJ USA
                Article
                10.1002/2017GL076901
                7cb1a0f9-9e1d-4924-989f-6dfac574c111
                © 2018

                http://creativecommons.org/licenses/by-nc-nd/4.0/

                http://doi.wiley.com/10.1002/tdm_license_1.1

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