, Das2 est un serveur conçu et utilisé par le groupe d'ondes radio et plasma de l'Université d'Iowa. Il permet, avec format das2stream, de distribuer les données aux utilisateur via un client (Autoplot par exemple), qui peut ensuite les visualiser et les manipuler
, Virtual European Solar and Planetary Access
, Analyses et Simulations d'Emissions Radio
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ADS -Detection of Jupiter decametric emissions controlled by Europa and Ganymede with Voyager, H.1.1 Premier auteur -Io-Jupiter decametric arcs observed by Juno/Waves compared to ExPRES simulations, vol.44, pp.9229-9247, 2017. ,
en préparation pour soumission à Geophysical Research Letters H.1.2 Co-auteur -Radio emission from satellite-Jupiter interactions (especially Ganymede), ADS -Location of the different jovian auroral radio sources using Juno / Waves, vol.618, pp.505-514, 2017. ,
en préparation pour soumission à Astronomy & Astrophysics -Probing Jovian broadband kilometric radio sources tied to the ultraviolet main auroral oval with Juno, soumis pour publication à Geophysical Research Letters H.2 Conferences 2017 ExPRES simulations of Jupiter-satellite decametric emissions : a parametric study, 2017. ,
Louis and 11 co-authors : -Oral at the Magnetospheres of the Outer Planets -Uppsala, Sweden -Oral at the Plas@par young reasearcher's day -Paris, France -Oral at the SF2A conference, P. Zarka Poster at the PNST conference, 2015. ,
, Team meetings 2016-2018 Participations fréquentes au Juno magnetospheric working group -à distance 2018 Juno science team meeting -Boudler, USA 2017 Juno science team meeting -New Orleans, USA 2017 Sakura team meeting
, USA 2016 Sakura team meeting -Vienna, Austria 2015 Working group LESIA-IRAP -Toulouse
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, A PARAMETRIC STUDY
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Model of Jovian magnetic field topology constrained by the Io auroral emissions, J. Geophys. Res, vol.116, p.5217, 2011. ,
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, Generation of the Jovian hectometric radiation: first lessons from Juno, vol.44, pp.4439-4446, 2017.
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, J. Geophys. Res. Space Physics, vol.122, pp.9228-9247, 2017.
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, ONERA
, The Juno spacecraft, Jupiter orbit since, 2016.
, MHz with the Waves experiment. The Waves data used in this paper are recorded continuously at low time-frequency (t-f) resolutions acquired in "survey" mode
These radio emissions are produced via the Cyclotron Maser Instability (CMI) by electrons with keV (possibly up to 10 s of keV) typical energy, gained through acceleration along magnetic field lines above the auroral regions or along magnetic flux tubes connecting Galilean satellites to Jupiter, mainly Io, but also Ganymede and Europa, In the decametric (DAM) wavelength range, Jupiter's radio emission is structured in the form of discrete arcs in the t-f plane, labeled "A" when the radio source is located in the north-right of Jupiter, 1983. ,
This angle is computed in a self-consistent way (ignoring refraction) in the frame of the CMI theory based on the choice of the electron distribution that drives the emission: loss cone distribution produces oblique emission with variable ?(f), whereas ring/shell distribution produces perpendicular emission (? ~ 90°) at all frequencies, 2008. ,
, First Juno/Waves observations compared to ExPRES simulations of Jupiter-Io decametric emission ? Near equator ExPRES simulations show that most of the arcs observed in the time-frequency plane by Juno, Wind, and Nançay are due to Io ? The simulations and observations of Io arcs are in good agreement when the modeled radio beaming angle ?, Special Section: Early Results: Juno at Jupiter Key Points: ?, pp.70-75
Io-Jupiter decametric arcs observed by Juno/Waves compared to ExPRES simulations, Supporting Information: ? Supporting Information S1 Correspondence to: C. K. Louis, corentin.louis@obspm.fr Citation: Louis, vol.44, pp.9225-9232, 2017. ,
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