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Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/1886
DC FieldValueLanguage
dc.contributor.authorallKecic, K. J.; Geomagnetic Institute, Grocka, Belgrade, Yugoslaviaen
dc.contributor.authorallBradley, P. A.; Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K.en
dc.contributor.authorallCander, L. R.; Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K.en
dc.contributor.authorallDick, M. I.; Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K.en
dc.contributor.authorallZolesi, B.; Istituto Nazionale di Geofisica, Roma, ItalyIstituto Nazionale di Geofisica, Roma, Italyen
dc.date.accessioned2006-12-06T11:20:43Zen
dc.date.available2006-12-06T11:20:43Zen
dc.date.issued1994-05en
dc.identifier.urihttp://hdl.handle.net/2122/1886en
dc.description.abstractThe present study discusses and compares the IRI and DGR ionospheric models using N(h) profiles obtained during a high solar activity period at South Uist ionosonde station. After inversion, N(h) profiles obtained from ionograms at South Uist have been compared with those derived from the IRI-90 and DGR ionospheric models. A small data set has been selected such that both geomagnetically quiet and disturbed conditions are represented. The importance of further comparisons with additional sets of N(h) profiles under different solar-geophysical conditions and at more stations has been recognized.en
dc.format.extent2956765 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.relation.ispartofseries2/37 (1994)en
dc.subjectIonosphereen
dc.subjectelectron density modelsen
dc.subjectheight profilesen
dc.subjecttestingen
dc.subjectmodel comparisonen
dc.titleFurther tests of the IRI and DGR model ionospheresen
dc.typearticleen
dc.type.QualityControlPeer-revieweden
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorKecic, K. J.en
dc.contributor.authorBradley, P. A.en
dc.contributor.authorCander, L. R.en
dc.contributor.authorDick, M. I.en
dc.contributor.authorZolesi, B.en
dc.contributor.departmentGeomagnetic Institute, Grocka, Belgrade, Yugoslaviaen
dc.contributor.departmentRutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K.en
dc.contributor.departmentRutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K.en
dc.contributor.departmentRutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K.en
dc.contributor.departmentIstituto Nazionale di Geofisica, Roma, ItalyIstituto Nazionale di Geofisica, Roma, Italyen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptGeomagnetic Institute, Grocka, Belgrade, Yugoslavia-
crisitem.author.deptRutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K.-
crisitem.author.deptRutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K.-
crisitem.author.deptRutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0002-7263-5043-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
Appears in Collections:Annals of Geophysics
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