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Corotation Plasma Environment Model : An Empirical Probability Model of the Jovian Magnetosphere

Futaana, Yoshifumi (author)
Swedish Inst Space Phys, SE-98128 Kiruna, Sweden
Wang, Xiao-Dong (author)
Swedish Inst Space Phys, Solar Syst Phys & Space Technol Grp, SE-98128 Kiruna, Sweden
Roussos, Elias (author)
Max Planck Inst Solar Syst Res, D-37077 Gottingen, Germany
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Krupp, Norbert (author)
Wahlund, Jan-Erik (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Ågren, Karin, 1980- (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Fränz, Markus (author)
Barabash, Stas (author)
Swedish Inst Space Phys, SE-98128 Kiruna, Sweden
Lei, Fan (author)
RadMod Res Ltd, Camberley GU15 2PD, England
Heynderickx, Daniel (author)
DH Consultancy BVBA, B-3000 Leuven, Belgium
Truscott, Pete (author)
Kallisto Consultancy Ltd, Farnborough GU14 9AJ, Hants, England
Cipriani, Fabrice (author)
European Space Agcy, European Space Res & Technol Ctr, NL-2200 AG Noordwijk, Netherlands
Rodgers, David (author)
European Space Agcy, European Space Res & Technol Ctr, NL-2200 AG Noordwijk, Netherlands
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 (creator_code:org_t)
IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC, 2018
2018
English.
In: IEEE Transactions on Plasma Science. - : IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC. - 0093-3813 .- 1939-9375. ; 46:6, s. 2126-2145
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We developed a new empirical model for corotating plasma in the Jovian magnetosphere. The model, named the corotation plasma environment model version 2 (CPEMv2), considers the charge density, velocity vector, and ion temperature based on Galileo/plasma system (PLS) ion data. In addition, we develop hot electron temperature and density models based on Galileo/PLS electron data. All of the models provide respective quantities in the magnetic equator plane of 9-30RJ, while the charge density model can be extended to 3-D space. A characteristic feature of the CPEM is its support of the percentile as a user input. This feature enables us to model extreme conditions in addition to normal states. In this paper, we review the foundations of the new empirical model, present a general derivation algorithm, and offer a detailed formulation of each parameter of the CPEMv2. As all CPEM parameters are of the analytical form, their implementation is straightforward, and execution involves the use of a small number of computational resources. The CPEM is flexible; for example, it can be extended, as new data (from observations or simulation results) become available. The CPEM can be used for the mission operation of the European Space Agency's mission to Jupiter, JUpiter ICy moons Explorer (JUICE), and for future data analyses.

Subject headings

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

Keyword

Corotation plasma
empirical model
Jupiter magnetosphere

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