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dc.contributor.authorCaro Carretero, Raqueles-ES
dc.contributor.authorCao, Y-Tes-ES
dc.contributor.authorWellbrock, A.es-ES
dc.date.accessioned2019-12-11T14:49:36Z
dc.date.available2019-12-11T14:49:36Z
dc.date.issued06/01/2020es_ES
dc.identifier.issn0148-0227es_ES
dc.identifier.uri10.1029/2019JE006252es_ES
dc.descriptionArtículos en revistases_ES
dc.description.abstractThe ionization of N2 by strong solar He II 30.4 nm photons produces distinctive spectral 22 peaks near 24.1 eV in Titan s upper atmosphere, which have been observed by the Elec23 tron Spectrometer (ELS) as part of the Cassini Plasma Spectrometer (CAPS). The ELS observations reveal that, in addition to the dayside, photoelectron peaks were also detected on the deep nightside where photoionization is switched off, as well as at sufficiently high altitudes where the ambient neutral density is low.es-ES
dc.description.abstractThe ionization of N2 by strong solar He II 30.4 nm photons produces distinctive spectral peaks near 24.1 eV in Titan s upper atmosphere, which have been observed by the Electron Spectrometer (ELS) as part of the Cassini Plasma Spectrometer (CAPS). The ELS observations reveal that, in addition to the dayside, photoelectron peaks were also detected on the deep nightside where photoionization is switched off, as well as at sufficiently high altitudes where the ambient neutral density is low. These photoelectron peaks are unlikely to be produced locally but instead must be contributed by transport along the magnetic field lines from their dayside source regions. In this study, we present a statistical survey of all photoelectron peaks identified with an automatic finite impulse response algorithm based on the available ELS data accumulated during 56 Titan flybys.en-GB
dc.format.mimetypeapplication/pdfes_ES
dc.language.isoes-ESes_ES
dc.rightses_ES
dc.rights.uries_ES
dc.sourceRevista: Journal of Geophysical Research, Periodo: 12, Volumen: , Número: , Página inicial: 1, Página final: 25es_ES
dc.titleField-aligned photoelectron energy peaks at high altitude and on the nightside of Titan JGR-IMPACT FACTOR. 3,71 https://agupubs.onlinelibrary.wiley.com/journal/21699100 ISSN 2169-9100es_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.description.versioninfo:eu-repo/semantics/publishedVersiones_ES
dc.rights.holderdisponible onlinees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/restrictedAccesses_ES
dc.keywordsTitan flybyses-ES
dc.keywordsTitan flybys, photoelectronsen-GB
dc.identifier.doi10.1029/2019JE006252es_ES


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