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dc.contributorSchool of Cosmic Physics, DIAS Dunsink Observatory, Dublin Institute for Advanced Studies, Dublin 15, Ireland; Station de Radioastronomie de Nançay, Observatoire de Paris, PSL Research University, CNRS, Université d'Orléans, F-18330 Nançay, France
dc.contributorSchool of Cosmic Physics, DIAS Dunsink Observatory, Dublin Institute for Advanced Studies, Dublin 15, Ireland
dc.contributorStation de Radioastronomie de Nançay, Observatoire de Paris, PSL Research University, CNRS, Université d'Orléans, F-18330 Nançay, France; LPC2E - Université d'Orléans/CNRS, 45071 Orléans, France
dc.contributorMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
dc.contributorSchool of Cosmic Physics, DIAS Dunsink Observatory, Dublin Institute for Advanced Studies, Dublin 15, Ireland; School of Physics, Trinity College Dublin, Dublin, D02 PN40, Ireland
dc.contributorAstrophysics Research Group, School of Mathematics, Statistics and Applied Mathematics, National University of Ireland Galway, University Road, Galway, H91 H3CY, Ireland
dc.contributorAstrophysics Research Group, School of Mathematics, Statistics and Applied Mathematics, National University of Ireland Galway, University Road, Galway, H91 H3CY, Ireland; Armagh Observatory and Planetarium, College Hill, Armagh, BT61 9DB, N. Ireland
dc.contributorSchool of Physics, Trinity College Dublin, Dublin, D02 PN40, Ireland
dc.contributorDepartment of Physics, University College Cork, Cork, T12 CY82, Ireland
dc.contributorCentre for Astronomy, School of Physics, National University of Ireland Galway, University Road, Galway, H91 TK33, Ireland
dc.contributorLeibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany
dc.contributor.authorLouis, Corentin K.
dc.contributor.authorJackman, C. M.
dc.contributor.authorGrießmeier, J. -M.
dc.contributor.authorWucknitz, O.
dc.contributor.authorMcKenna, D. J.
dc.contributor.authorMurphy, P. C.
dc.contributor.authorGallagher, P. T.
dc.contributor.authorCarley, E. P.
dc.contributor.authorÓ Fionnagáin, D.
dc.contributor.authorGolden, A.
dc.contributor.authorMcCauley, J.
dc.contributor.authorCallanan, P.
dc.contributor.authorRedman, M.
dc.contributor.authorVocks, C.
dc.date.accessioned2024-02-21T11:03:12Z
dc.date.available2024-02-21T11:03:12Z
dc.date.issued2022-04-01T00:00:00Z
dc.identifier.doi10.1093/rasti/rzac005
dc.identifier.doi10.48550/arXiv.2111.09599
dc.identifier.other2021arXiv211109599L
dc.identifier.otherastro-ph.EP
dc.identifier.otherastro-ph.IM
dc.identifier.other10.48550/arXiv.2111.09599
dc.identifier.otherarXiv:2111.09599
dc.identifier.other2022RASTI...1...48L
dc.identifier.other2021arXiv211109599L
dc.identifier.other10.1093/rasti/rzac005
dc.identifier.other0000-0002-9552-8822
dc.identifier.other0000-0003-0635-7361
dc.identifier.other0000-0003-3362-7996
dc.identifier.other0000-0001-8348-4861
dc.identifier.other0000-0001-7185-1310
dc.identifier.other0000-0002-8606-2645
dc.identifier.other0000-0001-9745-0400
dc.identifier.other0000-0002-6106-5292
dc.identifier.other0000-0001-9747-3573
dc.identifier.other0000-0001-8208-4292
dc.identifier.other0000-0003-4399-2233
dc.identifier.other0000-0003-4194-5484
dc.identifier.other0000-0002-1021-9343
dc.identifier.other0000-0001-8583-8619
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1775
dc.description.abstractThe Low Frequency Array (LOFAR) is an international radio telescope array, consisting of 38 stations in the Netherlands and 14 international stations spread over Europe. Here, we present an observation method to study the Jovian decametric radio emissions from several LOFAR stations (here Birr Castle in Ireland, Nançay in France, and Postdam in Germany), at high temporal and spectral resolution. This method is based on prediction tools, such as radio emission simulations and probability maps, and data processing. We report an observation of Io-induced decametric emission from 2021 June, and a first case study of the substructures that compose the macroscopic emissions (called millisecond bursts). The study of these bursts makes it possible to determine the electron populations at the origin of these emissions. We then present several possible future avenues for study based on these observations. The methodology and study perspectives described in this paper can be applied to new observations of Jovian radio emissions induced by Io, but also by Ganymede or Europa, or Jovian auroral radio emissions.
dc.publisherRAS Techniques and Instruments
dc.titleMethod to observe Jupiter's radio emissions at high resolution using multiple LOFAR stations: a first case study of the Io-decametric emission using the Irish IE613, French FR606, and German DE604 stations
dc.typearticle
dc.source.journalRASTI
dc.source.journalRASTI...1
dc.source.volume1
refterms.dateFOA2024-02-21T11:03:12Z
dc.identifier.bibcode2022RASTI...1...48L


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