The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the BZ Component of Interplanetary Magnetic Field

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dc.authoridÜNAL, İbrahim/0000-0001-8497-4459;
dc.authorwosidÜNAL, İbrahim/ABH-5657-2020
dc.authorwosidTİMOÇİN, Erdinç/H-2855-2017
dc.contributor.authorTimocin, Erdinc
dc.contributor.authorYesil, Ali
dc.contributor.authorUnal, Ibrahim
dc.date.accessioned2024-08-04T20:47:22Z
dc.date.available2024-08-04T20:47:22Z
dc.date.issued2020
dc.departmentİnönü Üniversitesien_US
dc.description.abstractIn this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the B-Z component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity (sigma(0)), Pedersen conductivity (sigma(1)), Hall conductivity (sigma(2)) data calculated for Rome (41.8 degrees N, 12.5 degrees E); Juliusruh (54.6 degrees N, 13.4 degrees E); Uppsala (59.8 degrees N, 17.6 degrees E); Lycksele (64.7 degrees N, 18.8 degrees E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the B-Z component. From the analysis results it is observed that the turnings in the B-Z component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the B-Z component increases all conductivities while the northward turnings of the B-Z component decreases all conductivities. The effect on the conductivities of the changes in the B-Z component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the B-Z component as latitude increase.en_US
dc.identifier.doi10.1007/s11277-020-07510-z
dc.identifier.endpage2932en_US
dc.identifier.issn0929-6212
dc.identifier.issn1572-834X
dc.identifier.issue4en_US
dc.identifier.scopus2-s2.0-85085653450en_US
dc.identifier.scopusqualityQ2en_US
dc.identifier.startpage2923en_US
dc.identifier.urihttps://doi.org/10.1007/s11277-020-07510-z
dc.identifier.urihttps://hdl.handle.net/11616/99324
dc.identifier.volume114en_US
dc.identifier.wosWOS:000536741400004en_US
dc.identifier.wosqualityQ4en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.ispartofWireless Personal Communicationsen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectIonosphereen_US
dc.subjectIonospheric conductivitiesen_US
dc.subjectInterplanetary magnetic fielden_US
dc.subjectSuperposed epoch analysisen_US
dc.titleThe Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the BZ Component of Interplanetary Magnetic Fielden_US
dc.typeArticleen_US

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