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dc.contributor.authorToledo Redondo, Sergio
dc.contributor.authorSalinas Extremera, Alfonso 
dc.contributor.authorPorti Durán, Jorge Andrés 
dc.contributor.authorWitasse, O.
dc.contributor.authorCardnell, S.
dc.contributor.authorFornieles Callejón, Jesús Francisco 
dc.contributor.authorMolina Cuberos, Gregorio José
dc.contributor.authorDéprez, G.
dc.contributor.authorMontmessin, F.
dc.date.accessioned2019-12-12T12:00:01Z
dc.date.available2019-12-12T12:00:01Z
dc.date.issued2017-01-17
dc.identifier.citationToledo-Redondo, S., A. Salinas, J. Portí, O. Witasse, S. Cardnell, J. Fornieles, G. J. Molina-Cuberos, G. Déprez, and F. Montmessin (2017), Schumann resonances at Mars: Effects of the day-night asymmetry and the dust-loaded ionosphere, Geophys. Res. Lett., 44, 648–656, [doi:10.1002/2016GL071635]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/58274
dc.descriptionOwing to the large size of the dataset, scientists interested in it are encouraged to contact the authors directly. The atmospheric properties used in the present study have been taken from the Mars Climate Database http://www-mars.lmd.jussieu.fr/.es_ES
dc.description.abstractSchumann resonances are standing waves that oscillate in the electromagnetic cavity formed between the conducting lower ionosphere and the surface of the planet. They have been measured in situ only on Earth and Titan, although they are believed to exist on other planets like Mars. We report numerical simulations of the Martian electromagnetic cavity, accounting for the day-night asymmetry and different dust scenarios. It has been found that the resonances are more energetic on the nightside, the first resonance is expected to be 9–14 Hz depending on the dust activity and to have low quality factors (Q ≃ 2). This work serves as an input for the upcoming Exomars surface platform (launch 2020), who will attempt to measure them for the first time.es_ES
dc.description.sponsorshipThis work was supported by the Ministerio de Economía y Competitividad of Spain under the project with reference FIS2013-44975-P, cofinanced with FEDER funds of the European Union. S.T.R. holds an ESA research fellowship and acknowledges support from the ESA science faculty of the European Space Astronomy Centre (ESAC).es_ES
dc.language.isoenges_ES
dc.publisherWileyes_ES
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.titleSchumann resonances at Mars: Effects of the day-night asymmetry and the dust-loaded ionospherees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1002/2016GL071635


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Atribución-NoComercial-SinDerivadas 3.0 España
Except where otherwise noted, this item's license is described as Atribución-NoComercial-SinDerivadas 3.0 España