Ganymede's Ionosphere Observed by a Dual‐Frequency Radio Occultation With Juno

In June 2021, the Juno spacecraft executed a close flyby of Ganymede. During the encounter, Juno passed behind Ganymede for 15 min as observed from Earth, providing the geometry to conduct a radio occultation experiment to probe Ganymede's tenuous ionosphere. X‐band and Ka‐band radio links were transmitted from Juno to antennas at the Deep Space Network. Electrons encountered along the radio propagation path advance the signal's phase and a linear combination the two frequencies allows for a direct measurement of the electron content along the propagation path. On occultation ingress, an ionosphere peak of 2,000 ± 500 (1‐σ) cm−3 near the surface was observed. On occultation egress, no statistically significant ionosphere was detected. Ingress observation viewed where Ganymede's intrinsic magnetic field lines are open whereas egress observation viewed where the field lines are closed, implying electron impact ionization plays a key role in the generation of the ionosphere.

[1]  J. Connerney,et al.  Ganymede MHD Model: Magnetospheric Context for Juno's PJ34 Flyby , 2022, Geophysical Research Letters.

[2]  Ryan S. Park,et al.  Gravity Field of Ganymede After the Juno Extended Mission , 2021, Geophysical Research Letters.

[3]  N. Ivchenko,et al.  A sublimated water atmosphere on Ganymede detected from Hubble Space Telescope observations , 2021, Nature Astronomy.

[4]  M. Kivelson,et al.  The Magnetosphere of Ganymede , 2021 .

[5]  P. Withers Revised predictions of uncertainties in atmospheric properties measured by radio occultation experiments , 2020, Advances in Space Research.

[6]  F. Leblanc,et al.  Constraining Ganymede's neutral and plasma environments through simulations of its ionosphere and Galileo observations , 2020, Icarus.

[7]  T. Nordheim,et al.  Surface composition and properties of Ganymede: Updates from ground-based observations with the near-infrared imaging spectrometer SINFONI/VLT/ESO , 2019, Icarus.

[8]  F. Leblanc,et al.  First 3D test particle model of Ganymede's ionosphere , 2019, Icarus.

[9]  P. Dalba,et al.  Cassini Radio Occultation Observations of Titan's Ionosphere: The Complete Set of Electron Density Profiles , 2019, Journal of Geophysical Research: Space Physics.

[10]  W. Folkner,et al.  The Juno Gravity Science Instrument , 2017 .

[11]  P. Withers,et al.  Radio occultations of the Io plasma torus by Juno are feasible , 2017, 1701.07435.

[12]  P. J. Schinder,et al.  A numerical technique for two‐way radio occultations by oblate axisymmetric atmospheres with zonal winds , 2015 .

[13]  Sami W. Asmar,et al.  Detecting High Dynamics Signals From Open-Loop Radio Science Investigations , 2011, Proceedings of the IEEE.

[14]  R. Beebe Jupiter: The Planet, Satellites and Magnetosphere , 2005 .

[15]  Luciano Iess,et al.  Spacecraft Doppler tracking: Noise budget and accuracy achievable in precision radio science observations , 2005 .

[16]  A. Nagy,et al.  The ionospheres of Europa, Ganymede, and Callisto , 2001 .

[17]  Vytenis M. Vasyliūnas,et al.  The ionosphere of Ganymede , 2001 .

[18]  David P. Hinson,et al.  Initial results from radio occultation measurements with Mars Global Surveyor , 1999 .

[19]  Paul D. Feldman,et al.  The Far-Ultraviolet Oxygen Airglow of Europa and Ganymede , 1998 .

[20]  Steven Peter Joy,et al.  The magnetic field and magnetosphere of Ganymede , 1997 .

[21]  A. Kliore,et al.  The neutral atmosphere of Venus as studied with the Mariner V radio occultation experiments , 1971 .

[22]  J. W. Marini,et al.  The Effect of Satellite Spin on Two-Way Doppler Rangerate Measurements , 1971, IEEE Transactions on Aerospace and Electronic Systems.

[23]  G. Fjeldbo,et al.  The atmosphere of mars analyzed by integral inversion of the Mariner IV occultation data , 1968 .

[24]  D. Anderson,et al.  On the radio occultation method for studying planetary atmospheres , 1968 .

[25]  G S Levy,et al.  Occultation Experiment: Results of the First Direct Measurement of Mars's Atmosphere and Ionosphere , 1965, Science.

[26]  G. Fjeldbo,et al.  The bistatic radar‐occultation method for the study of planetary atmospheres , 1965 .

[27]  Calvin W.M Surface composition and properties of Ganymede : Updates from ground-based observations with the near-infrared imaging spectrometer , 2019 .

[28]  A. Kliore Satellite Atmospheres and Magnetospheres , 1998 .