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  5. A Preliminary Study of Magnetosphere-Ionosphere-Thermosphere Coupling at Jupiter: Juno Multi-Instrument Measurements and Modeling Tools
 

A Preliminary Study of Magnetosphere-Ionosphere-Thermosphere Coupling at Jupiter: Juno Multi-Instrument Measurements and Modeling Tools

Journal
JOURNAL OF GEOPHYSICAL RESEARCH. SPACE PHYSICS  
Date Issued
2021
Author(s)
Wang, Yuxian
•
Blanc, Michel
•
Louis, Corentin
•
Wang, Chi
•
André, Nicolas
•
ADRIANI, Alberto  
•
Allegrini, Frederic
•
Blelly, Pierre-Louis
•
Bolton, Scott
•
Bonfond, Bertrand
•
Clark, George
•
Dinelli, Bianca Maria
•
Gérard, Jean-Claude
•
Gladstone, Randy
•
Grodent, Denis
•
Kotsiaros, Stavros
•
Kurth, William
•
Lamy, Laurent
•
Louarn, Philippe
•
Marchaudon, Aurélie
•
Mauk, Barry
•
MURA, Alessandro  
•
Tao, Chihiro
DOI
10.1029/2021JA029469
Abstract
The dynamics of the Jovian magnetosphere are controlled by the interplay of the planet's fast rotation, its main iogenic plasma source and its interaction with the solar wind. Magnetosphere-Ionosphere-Thermosphere (MIT) coupling processes controlling this interplay are significantly different from their Earth and Saturn counterparts. At the ionospheric level, they can be characterized by a set of key parameters: ionospheric conductances, electric currents and fields, exchanges of particles along field lines, Joule heating and particle energy deposition. From these parameters, one can determine (a) how magnetospheric currents close into the ionosphere, and (b) the net deposition/extraction of energy into/out of the upper atmosphere associated to MIT coupling. We present a new method combining Juno multi-instrument data (MAG, JADE, JEDI, UVS, JIRAM and Waves) and modeling tools to estimate these key parameters along Juno's trajectories. We first apply this method to two southern hemisphere main auroral oval crossings to illustrate how the coupling parameters are derived. We then present a preliminary statistical analysis of the morphology and amplitudes of these key parameters for eight among the first nine southern perijoves. We aim to extend our method to more Juno orbits to progressively build a comprehensive view of Jovian MIT coupling at the level of the main auroral oval.
Volume
126
Issue
9
Start page
e29469
Uri
http://hdl.handle.net/20.500.12386/36829
Url
https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2021JA029469
https://api.elsevier.com/content/abstract/scopus_id/85115750266
Issn Identifier
2169-9380
Ads BibCode
2021JGRA..12629469W
Rights
open.access
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