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dc.contributor.authorAfraimovich, E.L.
dc.contributor.authorAstafieva, E.I.
dc.contributor.authorVoeykov, S.V.
dc.contributor.authorTsegmed, B.
dc.contributor.authorPotekhin, A.P.
dc.contributor.authorRasson,J.L.
dc.coverage.temporal21st century
dc.date2006
dc.date.accessioned2016-03-07T16:16:52Z
dc.date.accessioned2021-12-09T09:53:39Z
dc.date.available2016-03-07T16:16:52Z
dc.date.available2021-12-09T09:53:39Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/8714
dc.descriptionComparative analysis of total electron content (TEC) variations and geomagnetic field variations during the major magnetic storm on 29-31 October 2003 (Kp 4-9) was carried out for the middle-latitude ionosphere. We analyzed data of GPS receivers and magnetic observatories, located in the north-east, north-west and south-west parts of North America and in central Europe. It was found that magnetic field intensity variations for the period range of 30-60 min (corresponding to the acoustic-gravity waves, AGWs) correlate well with TEC variations of the same time scale. For moderate geomagnetic activity period on October 13-18, 1999 (Kp 1-A) a similar dependence was not noticed, according to analysis of data from GPS receivers located in south-west USA, California. However, correlation between TEC variation intensity in the period range of 30-60 min and slow magnetic field changes was observed. Thus, connection between TEC variations within the period range of the AGWs and magnetic field variations is perceptible.
dc.languageeng
dc.publisherIRM
dc.publisherKMI
dc.publisherRMI
dc.relation.ispartofseriesAdvances in Space Research V 38
dc.titleAn investigation of the correlation between ionospheric and geomagnetic variations using data from the GPS and INTERMAGNET networks
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceGeneral Public
dc.audienceScientific
dc.subject.freeIonosphere
dc.subject.freeGPS
dc.subject.freeINTERMAGNET
dc.subject.freeGeomagnetic variations
dc.subject.freeTEC variations
dc.source.issueAdvances in Space Research V 38
dc.source.pagep. 2332-2336
Orfeo.peerreviewedNot pertinent


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