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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Discussion papers | Copyright
https://doi.org/10.5194/angeo-2018-82
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

Regular paper 12 Jul 2018

Regular paper | 12 Jul 2018

Review status
This discussion paper is a preprint. It is a manuscript under review for the journal Annales Geophysicae (ANGEO).

Analysis of Juno perijove 1 magnetic field data using the Jovian paraboloid magnetospheric model

Ivan A. Pensionerov1, Elena S. Belenkaya1, Stanley W. H. Cowley2, Igor I. Alexeev1, Vladimir V. Kalegaev1, and David A. Parunakian1 Ivan A. Pensionerov et al.
  • 1Federal State Budget Educational Institution of Higher Education M.V. Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU), 1(2), Leninskie gory, GSP-1, Moscow 119991, Russian Federation
  • 2Department of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UK

Abstract. One of the main features of Jupiter's magnetosphere is its equatorial magnetodisc, which significantly increases the field strength and size of the magnetosphere. Juno measurements of the magnetic field during the perijove 1 pass have allowed us to determine optimal parameters of the magnetodisc using the paraboloid magnetospheric magnetic field model, which employs analytic expressions for the magnetospheric current systems. Specifically within the model we determine the size of the Jovian magnetodisc and the magnetic field strength at its outer edge.

Ivan A. Pensionerov et al.
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Ivan A. Pensionerov et al.
Ivan A. Pensionerov et al.
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Short summary
In the present work we used unique data on the magnetic field in the Jovian magnetosphere measured by the Juno spacecraft. The data allowed us to determine optimal parameters of the magnetodisc in the paraboloid magnetospheric model and find the ways to qualitatively improve the model.
In the present work we used unique data on the magnetic field in the Jovian magnetosphere...
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