Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/1264
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dc.contributor.authorallDe Franceschi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallGulyaeva, T. L.; IZMIRAN, Russian Academy of Sciences, Troitsk, Moscow Region, Russiaen
dc.contributor.authorallPerrone, L.; Space Research Centre, PAS, Warsaw, Polanden
dc.date.accessioned2006-07-05T08:11:27Zen
dc.date.available2006-07-05T08:11:27Zen
dc.date.issued2001-10en
dc.identifier.urihttp://hdl.handle.net/2122/1264en
dc.description.abstractAn attempt at forecasting the magnetic activity index three hours in advance is presented. This approach is based on a suitable treatment of time-weighted accumulations of the three-hourly magnetic index Kp. The statistical analysis of impact of magnetic activity on the positive and negative disturbances of the F 2 layer peak electron density NmF 2 is made for 25 ionosondes in Europe and Russia during 1997 to 2001. It is shown that the response of positive and negative ionosphere disturbances to peak of magnetic activity Kpmax delays by 1 to 48 h. Two peaks of occurrence of positive and negative ionospheric disturbed periods are found referring to Kpmax equal to 3 and 4 for DNmF2+ and Kpmax equal to 4 and 5 for DNmF2– shifted regarding similar distribution of forecasted Kpm indices depicting two maxima at Kp equal to 1.7 and 2.7. Comparisons are made with observations and IRI-2001 model predictions.en
dc.format.extent2915522 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.relation.ispartofseries5-6/44 (2001)en
dc.subjectGeomagnetic activityen
dc.subjectionospheric disturbanceen
dc.subjectferecastingen
dc.titleForecasting geomagnetic activity three hours in advance for ionospheric applicationsen
dc.typearticleen
dc.type.QualityControlPeer-revieweden
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.03. Forecastsen
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.99. General or miscellaneousen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorDe Franceschi, G.en
dc.contributor.authorGulyaeva, T. L.en
dc.contributor.authorPerrone, L.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIZMIRAN, Russian Academy of Sciences, Troitsk, Moscow Region, Russiaen
dc.contributor.departmentSpace Research Centre, PAS, Warsaw, Polanden
item.openairetypearticle-
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.deptIzmiran Russian Academy of Sciences, Troitsk, Moscow Region, Russia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0002-3943-6798-
crisitem.author.orcid0000-0003-4335-0345-
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.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
Appears in Collections:Annals of Geophysics
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