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dc.contributor.authorProl, Fabricio dos Santos
dc.contributor.authorHernández Pajares, Manuel
dc.contributor.authorHonorato Muella, Marcio Tadeu de Assis
dc.contributor.authorCamargo, Paulo de Oliveira
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Matemàtiques
dc.date.accessioned2018-12-11T09:35:03Z
dc.date.available2018-12-11T09:35:03Z
dc.date.issued2018-10-01
dc.identifier.citationProl, F., Hernandez, M., Honorato, M., Camargo, P. Tomographic imaging of ionospheric plasma bubbles based on GNSS and radio occultation measurements. "Remote sensing", 1 Octubre 2018, vol. 10, núm. 10, p. 1-16.
dc.identifier.issn2072-4292
dc.identifier.urihttp://hdl.handle.net/2117/125602
dc.description.abstractTotal electron content measurements given by the global navigation satellite system (GNSS) have successfully presented results to capture the signatures of equatorial plasma bubbles. In contrast, the correct reproduction of plasma depletions at electron density level is still a relevant challenge for ionospheric tomographic imaging. In this regard, this work shows the first results of a new tomographic reconstruction technique based on GNSS and radio-occultation data to map the vertical and horizontal distributions of ionospheric plasma bubbles in one of the most challenging conditions of the equatorial region. Twenty-three days from 2013 and 2014 with clear evidence of plasma bubble structures propagating through the Brazilian region were analyzed and compared with simultaneous observations of all-sky images in the 630.0 nm emission line of the atomic oxygen. The mean rate of success of the tomographic method was 37.1%, being more efficient near the magnetic equator, where the dimensions of the structures are larger. Despite some shortcomings of the reconstruction technique, mainly associated with ionospheric scintillations and the weak geometry of the ground-based GNSS receivers, both vertical and horizontal distributions were mapped over more than 30° in latitude, and have been detected in instances where the meteorological conditions disrupted the possibility of analyzing the OI 630 nm emissions. Therefore, the results revealed the proposed tomographic reconstruction as an efficient tool for mapping characteristics of the plasma bubble structures, which may have a special interest in Space Weather, Spatial Geodesy, and Telecommunications.
dc.format.extent16 p.
dc.language.isoeng
dc.publisherMultidisciplinary Digital Publishing Institute (MDPI)
dc.subjectÀrees temàtiques de la UPC::Matemàtiques i estadística::Matemàtica aplicada a les ciències
dc.subjectÀrees temàtiques de la UPC::Matemàtiques i estadística
dc.subject.lcshGeophysics
dc.subject.lcshAstronomy and astrophysics
dc.subject.otherequatorial ionosphere
dc.subject.otherplasma bubble detection
dc.subject.othertotal electron content mapping
dc.subject.othermultiplicative algebraic reconstruction technique
dc.subject.otheroptical imaging
dc.subject.other630.0 nm emission line
dc.titleTomographic imaging of ionospheric plasma bubbles based on GNSS and radio occultation measurements
dc.typeArticle
dc.subject.lemacGeofísica
dc.subject.lemacAstrofísica
dc.contributor.groupUniversitat Politècnica de Catalunya. IonSAT - Grup de determinació Ionosfèrica i navegació per SAtèl·lit i sistemes Terrestres
dc.identifier.doi10.3390/rs10101529
dc.description.peerreviewedPeer Reviewed
dc.subject.amsClassificació AMS::86 Geophysics
dc.subject.amsClassificació AMS::85 Astronomy and astrophysics
dc.relation.publisherversionhttps://www.mdpi.com/2072-4292/10/10/1529
dc.rights.accessOpen Access
drac.iddocument23512052
dc.description.versionPostprint (published version)
upcommons.citation.authorProl, F.; Hernandez, M.; Honorato, M.; Camargo, P.
upcommons.citation.publishedtrue
upcommons.citation.publicationNameRemote sensing
upcommons.citation.volume10
upcommons.citation.number10
upcommons.citation.startingPage1
upcommons.citation.endingPage16


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