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Showing 1–6 of 6 results
Advanced filters: Author: B. Bonfond Clear advanced filters

  • The detection of the auroral footprint of Jupiter’s moon Callisto is challenging, but a shift in Jupiter’s bright main auroral oval could provide an opportunity for potential detections. Here, the authors show observation of the ultraviolet footprint of Callisto using Juno spacecraft data, benefiting from such opportunity.

    • J. Rabia
    • V. Hue
    • S. J. Bolton
    ResearchOpen Access
    Nature Communications
    Volume: 16, P: 1-12

  • Simulations show that the competing effects of the solar wind and planetary rotation can explain the structure of planetary aurorae: the former dominates for Earth-type and the latter for Jupiter-type aurorae, with the highly variable aurorae at Saturn representing a transition state.

    • B. Zhang
    • Z. Yao
    • J. G. Lyon
    Research
    Nature Astronomy
    Volume: 8, P: 964-972

  • Far-UV observations from the Hubble Space Telescope provide evidence of water vapour in the tenuous atmosphere of Ganymede. Atmospheric water originates from surface ice sublimation, with an enrichment in the subsolar region and substantial asymmetry between the leading and trailing hemispheres.

    • Lorenz Roth
    • Nickolay Ivchenko
    • Kurt D. Retherford
    Research
    Nature Astronomy
    Volume: 5, P: 1043-1051

  • An intensification of the 7.8-µm methane emission at Jupiter’s poles is observed in coincidence with the arrival of a solar-wind compression in January 2017, highlighting the strong coupling between Jupiter’s magnetosphere and its neutral stratosphere.

    • J. A. Sinclair
    • G. S. Orton
    • P. G. J. Irwin
    Research
    Nature Astronomy
    Volume: 3, P: 607-613

  • The authors discover that Jupiter's southern X-ray aurora is concentrated into a hot spot (until now only the north pole was known to have one), which behaves completely differently in brightness and timing pulsation from its northern counterpart.

    • W. R. Dunn
    • G. Branduardi-Raymont
    • A. J. Coates
    Research
    Nature Astronomy
    Volume: 1, P: 758-764