Survey of Juno Observations in Jupiter's Plasma Disk: Density
RESEARCH ARTICLE Survey of Juno Observations in Jupiter's Plasma Disk: 10.1029/2021JA029446 Density Key Points: E. Huscher1, F. Bagenal1 , R. J. Wilson1 , F. Allegrini2,3 , R. W. Ebert2,3 , P. W. Valek2 , • On most orbits, the densities exhibit J. R. Szalay4 , D. J. McComas4 , J. E. P. Connerney5,6 , S. Bolton2 , and S. M. Levin7 regular behavior mapping out a disk confined close to the centrifugal 1Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, USA, 2Southwest Research equator 3 • Small-scale ( minutes) variabilities Institute, San Antonio, TX, USA, Department of Physics and Astronomy, University of Texas at San Antonio, San 4 5 may indicate∼ radial transport via Antonio, TX, USA, Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA, Space Research local instabilities Corporation, Annapolis, MD, USA, 6Goddard Space Flight Center, Greenbelt, MD, USA, 7Jet Propulsion Laboratory/ • Occasionally a uniformly tenuous California Institute of Technology, Pasadena, CA, USA outer disk indicates enhanced losses, perhaps triggered by solar wind compression Abstract We explore the variation in plasma conditions through the middle magnetosphere of Jupiter with latitude and radial distance using Juno-JADE measurements of plasma density (electrons, protons, Supporting Information: sulfur, and oxygen ions) surveyed on Orbits 5–26 between March 2017 and April 2020. On most orbits, the Supporting Information may be found in the online version of this article. densities exhibit regular behavior, mapping out a disk between 10 and 50 RJ (Jovian radii). In the disk, the heavy ions are confined close to the centrifugal equator which oscillates relative to the spacecraft due to the 10° tilt of Jupiter's magnetic dipole.
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