Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/12682
DC FieldValueLanguage
dc.date.accessioned2019-08-26T07:15:37Zen
dc.date.available2019-08-26T07:15:37Zen
dc.date.issued2019-06en
dc.identifier.urihttp://hdl.handle.net/2122/12682en
dc.description.abstractIn this paper, a procedure for updating the International Reference Ionosphere (IRI) model by means of assimilated vertical total electron content (vTEC) measurements from a Global Navigational Satellite Systems (GNSS) receiver network is presented. This procedure stands as an additional implementation of the IRI UPdate (IRI UP) method, which is based on the assimilation of ionosonde derived F2 layer ionospheric characteristics. According to this, a mathematical procedure for obtaining foF2 and M(3000)F2 values from vTEC measurements is here proposed. Mathematical relationships between F2 layer characteristics and vTEC values have been derived using South African colocated ionosonde and GNSS stations. The same procedure can, however, be applied successfully in each region where such data are available. The goodness of the proposed IRI UP method, based on assimilated vTEC values, has been tested for several quiet and disturbed days in 2017 and 2018. IRI UP exhibits better performances than IRI for foF2, for most of the analyzed cases. Slight improvements are achieved in modeling hmF2 only for very disturbed periods in 2017. Due to the very good coverage of the terrestrial surface that GNSS receivers have achieved in recent years, we suggest that the method proposed here can be a good implementation of the IRI model for Space Weather nowcasting purposes, at least for foF2.en
dc.language.isoEnglishen
dc.relation.ispartofSpace Weatheren
dc.relation.ispartofseries/17 (2019)en
dc.titleOn the Development of a Method for Updating an Empirical Climatological Ionospheric Model by Means of Assimilated vTEC Measurements From a GNSS Receiver Networken
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1131-1164en
dc.identifier.doi10.1029/2019SW002185en
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeJCR Journalen
dc.contributor.authorPignalberi, Alessioen
dc.contributor.authorHabarulema, John Boscoen
dc.contributor.authorPezzopane, Michaelen
dc.contributor.authorRizzi, R.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentSouth African National Space Agency, Space Science, Hermanus, South Africaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentDipartimento di Fisica e Astronomia, Università di Bologna “Alma Mater Studiorum”, Bologna, Italyen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
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.deptSouth African National Space Agency, Space Science, Hermanus, South Africa-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptDipartimento di Fisica, Universita` di Bologna, Bologna, Italy-
crisitem.author.orcid0000-0001-9459-4919-
crisitem.author.orcid0000-0002-9716-7688-
crisitem.author.orcid0000-0001-5800-2322-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.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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