Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9959
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dc.contributor.authorallSpogli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallRomano, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallDe Franceschi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallAlfonsi, Lu.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallPlakidis, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallCesaroni, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallAquino, M.; University of Nottingham, Nottingham, UKen
dc.contributor.authorallDodson, A.; University of Nottingham, Nottingham, UKen
dc.contributor.authorallGalera Monico, J. F.; Departamento de Cartografia, Universidade Estadual Paulista Júlio de Mesquita Filho, Brazilen
dc.contributor.editorallNotarpietro, R.; Politecnico di Torinoen
dc.contributor.editorallDe Franceschi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.editorallDovis, F.; Politecnico di Torinoen
dc.date.accessioned2015-06-14T10:55:45Zen
dc.date.available2015-06-14T10:55:45Zen
dc.date.issued2014-07-17en
dc.identifier.isbn978-953-51-1642-en
dc.identifier.urihttp://hdl.handle.net/2122/9959en
dc.description.abstractTo study ionospheric scintillation on L-band radio signals, it is nowadays typical to acquire data with GNSS (Global Navigation Satellite System) receivers working at high frequency sampling rate (50-100 Hz). When dealing with such data, it is common to consider the contribution coming solely from observations at elevation angles, calculated from the receiver to the selected satellite, above an arbitrary threshold, typically 15-30°. Filtering out measurements made at low elevation angles helps keeping a high SNR (Signal to Noise Ratio) and eliminating non-ionospheric related effects, such as multipath. The downside of that well consolidated method is a reduction of the field of view spanned by the GNSS receiver antenna, and, if it is the case, of the whole network. This is not crucial for dense networks or well covered areas, but it can be in the case of not well covered regions, for logistics (e.g. forests, deserts, etc.) and/or environmental reasons (e.g. oceans). The loss of information in many applications could be meaningful. In this paper, we present a method to filter out spurious data based on an “outliers analysis” able to efficiently remove multipath affected measurements, reducing the data loss from 35-45% to 10-20%. It is based upon the Ground Based Scintillation Climatology (GBSC) and the station characterization based upon GBSC [5] is applied to the CIGALA1/ CALIBRA2 network in Brazil. The research shown herein was carried out in the context of the CALIBRA (http://www.calibra-ionosphere.net) project and exploits the CIGALA/ CALIBRA network in Brazil, to which the method was applied, enlarging the field of view and, then, improving the capability of inferring the dynamics of the low latitude ionosphere.en
dc.language.isoEnglishen
dc.relation.ispartofMitigation of Ionospheric Threats to GNSS: an Appraisal of the Scientific and Technological Outputs of the TRANSMIT Projecten
dc.subjectGNSSen
dc.subjectdata filteringen
dc.subjectmultipathen
dc.subjectionsopheric scintillationen
dc.subjectlow latitude ionosphereen
dc.titleA Filtering Method Developed to Improve GNSS Receiver Data Quality in the CALIBRA Projecten
dc.typebook chapteren
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber109-117en
dc.identifier.URLhttp://www.intechopen.com/books/mitigation-of-ionospheric-threats-to-gnss-an-appraisal-of-the-scientific-and-technological-outputs-of-the-transmit-project/a-filtering-method-developed-to-improve-gnss-receiver-data-quality-in-the-calibra-projecten
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillationsen
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.publisherInTechen
dc.description.fulltextopenen
dc.contributor.authorSpogli, L.en
dc.contributor.authorRomano, V.en
dc.contributor.authorDe Franceschi, G.en
dc.contributor.authorAlfonsi, Lu.en
dc.contributor.authorPlakidis, E.en
dc.contributor.authorCesaroni, C.en
dc.contributor.authorAquino, M.en
dc.contributor.authorDodson, A.en
dc.contributor.authorGalera Monico, J. F.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentUniversity of Nottingham, Nottingham, UKen
dc.contributor.departmentUniversity of Nottingham, Nottingham, UKen
dc.contributor.departmentDepartamento de Cartografia, Universidade Estadual Paulista Júlio de Mesquita Filho, Brazilen
dc.contributor.editorNotarpietro, R.en
dc.contributor.editorDe Franceschi, G.en
dc.contributor.editorDovis, F.en
dc.contributor.editordepartmentPolitecnico di Torinoen
dc.contributor.editordepartmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.editordepartmentPolitecnico di Torinoen
item.openairetypebook chapter-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptInstitute of Engineering Surveying and Space Geodesy (IESSG), Nottingham, UK-
crisitem.author.deptInstitute of Engineering Surveying and Space Geodesy (IESSG) - University of Nottingham-
crisitem.author.orcid0000-0003-2310-0306-
crisitem.author.orcid0000-0002-7532-4507-
crisitem.author.orcid0000-0002-3943-6798-
crisitem.author.orcid0000-0002-1806-9327-
crisitem.author.orcid0000-0003-2268-4389-
crisitem.author.orcid0000-0003-2733-4716-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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