Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10438
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dc.contributor.authorallPietrella, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallNava, B.; The Abdus Salam International Centre for Theoretical Physics Strada Costiera 11. I-34051, Trieste, Italyen
dc.contributor.authorallPezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallMigoya Orue, Y.; The Abdus Salam International Centre for Theoretical Physics Strada Costiera 11. I-34051, Trieste, Italyen
dc.contributor.authorallIppolito, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallScotto, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2017-01-19T07:06:34Zen
dc.date.available2017-01-19T07:06:34Zen
dc.date.issued2017-01en
dc.identifier.urihttp://hdl.handle.net/2122/10438en
dc.description.abstractWithin the framework of the AUSPICIO (AUtomatic Scaling of Polar Ionograms and Co-operative Ionospheric Observations) project, a limited sample of ionograms recorded mostly in 2001 and 2009, and to a lesser extent in 2006–07 and 2012–15, at the ionospheric observatories of Hobart and MacquarieIsland (mid-latitude), Comandante FerrazandLivingstoneIsland(high latitude),andCasey, Mawson, Davis and Scott Base (inside the Antarctic Polar Circle (APC)) were considered to study the capability of the NeQuick2 and IRI2012 models for predicting the behaviour of the ionosphere at mid- and high latitudes and over the Antarctic area. The applicability of NeQuick2 and IRI2012 was evaluated as i) climatological models taking as input the F 10.7 solar activity index and ii) assimilative models ingesting the foF2 and hmF2 measurements obtained from the electron density profiles provided bytheAdaptiveIonosphericProfiler(AIP). Thestatisticalanalysisresults reveal thatthe bestdescription of the ionosphere’s electron density is achieved when the AIP measurements are ingested into the NeQuick2 and IRI2012 models. Moreover, NeQuick2 performance is far better than IRI2012 performance outside the APC. Conversely, the IRI2012 model performs better than the NeQuick2 model inside the APC.en
dc.description.sponsorshipProgetto Nazionale Ricerche in Antartideen
dc.language.isoEnglishen
dc.relation.ispartofAntarctic Scienceen
dc.relation.ispartofseries3/29 (2017)en
dc.subjectadaptive ionospheric profileren
dc.subjectautoscalaen
dc.subjectdata ingestionen
dc.subjectroot mean square erroren
dc.titleNeQuick2 and IRI2012 models applied to mid and high latitudes, and the Antarctic ionosphereen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber265-276en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
dc.identifier.doi10.1017/S0954102016000602en
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.contributor.authorPietrella, M.en
dc.contributor.authorNava, B.en
dc.contributor.authorPezzopane, M.en
dc.contributor.authorMigoya Orue, Y.en
dc.contributor.authorIppolito, A.en
dc.contributor.authorScotto, C.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentThe Abdus Salam International Centre for Theoretical Physics Strada Costiera 11. I-34051, Trieste, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentThe Abdus Salam International Centre for Theoretical Physics Strada Costiera 11. I-34051, Trieste, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
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.deptThe Abdus Salam International Centre for Theoretical Physics Strada Costiera 11. I-34051, Trieste, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptThe Abdus Salam International Centre for Theoretical Physics Strada Costiera 11. I-34051, Trieste, Italy-
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.orcid0000-0001-9069-4090-
crisitem.author.orcid0000-0001-5800-2322-
crisitem.author.orcid0000-0001-5290-7235-
crisitem.author.orcid0000-0003-3823-127X-
crisitem.author.orcid0000-0002-9437-6775-
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.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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