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Callisto plasma interactions : Hybrid modeling including induction by a subsurface ocean

Lindkvist, Jesper (author)
Umeå universitet,Institutionen för fysik,Swedish Institute of Space Physics, Kiruna
Holmström, Mats (author)
Swedish Institute of Space Physics, Kiruna
Khurana, Krishan K. (author)
Department of Earth and Space Sciences, University of California, Los Angeles
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Fatemi, Shahab (author)
Space Sciences Laboratory, University of California, Berkeley
Barabash, Stas (author)
Swedish Institute of Space Physics, Kiruna
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 (creator_code:org_t)
2015
2015
English.
In: Journal of Geophysical Research - Space Physics. - 2169-9380 .- 2169-9402. ; 120:6, s. 4877-4889
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • By using a hybrid plasma solver (ions as particles and electrons as a fluid), we have modeled the interaction between Callisto and Jupiter's magnetosphere for variable ambient plasma parameters. We compared the results with the magnetometer data from flybys (C3, C9, and C10) by the Galileo spacecraft. Modeling the interaction between Callisto and Jupiter's magnetosphere is important to establish the origin of the magnetic field perturbations observed by Galileo and thought to be related to a subsurface ocean. Using typical upstream magnetospheric plasma parameters and a magnetic dipole corresponding to the inductive response inside the moon, we show that the model results agree well with observations for the C3 and C9 flybys, but agrees poorly with the C10 flyby close to Callisto. The study does support the existence of a subsurface ocean at Callisto.

Subject headings

NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Keyword

Callisto
plasma interaction
hybrid model
subsurface ocean
Galileo flyby
magnetosphere

Publication and Content Type

ref (subject category)
art (subject category)

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