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  • Lindkvist, Jesper, 1986-, et al. (author)
  • Ceres interaction with the solar wind
  • 2017
  • In: Geophysical Research Letters. - 0094-8276 .- 1944-8007. ; 44:5, s. 2070-2077
  • Journal article (peer-reviewed)abstract
    • The solar wind interaction with Ceres is studied for a high water vapor release from its surface using a hybrid model including photoionization. We use a water vapor production rate of 6 kg/s, thought to be due to subsurface sublimation, corresponding to a detection on 6 March 2013 by the Herschel Space Observatory. We present the general morphology of the plasma interactions, both close to Ceres and on a larger scale. Mass loading of water ions causes a magnetic pileup region in front of Ceres, where the solar wind deflects up to 15 ∘ and slows down by 15%. The global plasma interaction with Ceres is not greatly affected by the source location of water vapor nor on gravity, only on the production rate of water vapor. On a global scale, Ceres has a comet-like interaction with the solar wind with observable perturbations farther than 250 Ceres radii downstream of the body.
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Type of publication
journal article (1)
Type of content
peer-reviewed (1)
Author/Editor
Fatemi, Shahab (1)
Wieser, Martin (1)
Barabash, Stas (1)
Holmström, Mats (1)
Lindkvist, Jesper, 1 ... (1)
University
Umeå University (1)
Language
English (1)
Research subject (UKÄ/SCB)
Natural sciences (1)
Year
2017 (1)

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