Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10300
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dc.contributor.authorallEnell, C.-F.; EISCAT Scientific Association, Kiruna, Swedenen
dc.contributor.authorallKozlovsky, A.; Sodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finlanden
dc.contributor.authorallTurunen, T.; Sodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finlanden
dc.contributor.authorallUlich, T.; Sodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finlanden
dc.contributor.authorallVälitalo, S.; Sodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finlanden
dc.contributor.authorallScotto, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallPezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2016-04-27T08:52:39Zen
dc.date.available2016-04-27T08:52:39Zen
dc.date.issued2016-03-23en
dc.identifier.urihttp://hdl.handle.net/2122/10300en
dc.description.abstractThis paper presents a comparison between standard ionospheric parameters manually and automatically scaled from ionograms recorded at the high-latitude Sodankylä Geophysical Observatory (SGO, ionosonde SO166, 64.1° geomagnetic latitude), located in the vicinity of the auroral oval. The study is based on 2610 ionograms recorded during the period June–December 2013. The automatic scaling was made by means of the Autoscala software. A few typical examples are shown to outline the method, and statistics are presented regarding the differences between manually and automatically scaled values of F2, F1, E and sporadic E (Es) layer parameters. We draw the conclusions that: 1. The F2 parameters scaled by Autoscala, foF2 and M(3000)F2, are reliable. 2. F1 is identified by Autoscala in significantly fewer cases (about 50 %) than in the manual routine, but if identified the values of foF1 are reliable. 3. Autoscala frequently (30% of the cases) detects an E layer when the manual scaling process does not. When identified by both methods, the Autoscala E-layer parameters are close to those manually scaled, foE agreeing to within 0.4 MHz. 4. Es and parameters of Es identified by Autoscala are in many cases different from those of the manual scaling. Scaling of Es at auroral latitudes is often a difficult task.en
dc.language.isoEnglishen
dc.publisher.nameCopernicus Publications on behalf of the European Geosciences Unionen
dc.relation.ispartofGeoscientific Instrumentation Methods and Data Systemen
dc.relation.ispartofseries/5(2016)en
dc.subjectionogramen
dc.subjectautoscalingen
dc.subjectAutoscalaen
dc.subjectionosondeen
dc.titleComparison between manual scaling and Autoscala automatic scaling applied to Sodankylä Geophysical Observatory ionogramsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber53-64en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.subject.INGV05. General::05.07. Space and Planetary sciences::05.07.01. Solar-terrestrial interactionen
dc.subject.INGV05. General::05.07. Space and Planetary sciences::05.07.02. Space weatheren
dc.identifier.doi10.5194/gi-5-53-2016en
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeN/A or not JCRen
dc.description.fulltextopenen
dc.contributor.authorEnell, C.-F.en
dc.contributor.authorKozlovsky, A.en
dc.contributor.authorTurunen, T.en
dc.contributor.authorUlich, T.en
dc.contributor.authorVälitalo, S.en
dc.contributor.authorScotto, C.en
dc.contributor.authorPezzopane, M.en
dc.contributor.departmentEISCAT Scientific Association, Kiruna, Swedenen
dc.contributor.departmentSodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finlanden
dc.contributor.departmentSodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finlanden
dc.contributor.departmentSodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finlanden
dc.contributor.departmentSodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finlanden
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptEISCAT Scientific Association, Kiruna, Sweden-
crisitem.author.deptSodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finland-
crisitem.author.deptSodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finland-
crisitem.author.deptSodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finland-
crisitem.author.deptSodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finland-
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.orcid0000-0002-9437-6775-
crisitem.author.orcid0000-0001-5800-2322-
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.classification.parent05. General-
crisitem.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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