The effects of solar flares on the very low frequency signals recorded by super SID system

dc.contributor.authorCanyilmaz, M.
dc.contributor.authorGuzel, E.
dc.contributor.authorAkdogan, T.
dc.date.accessioned2026-08-12T17:17:07Z
dc.date.issued2016
dc.departmentFırat Üniversitesi
dc.description.abstractSolar flares cause sudden disturbances at the Earth's ionosphere. These effects are detected by the very low frequency (VLF), 3-30-kHz signals which are propagated at the Earth-ionosphere waveguide. The sudden changes on the time-dependent intensity of VLF signals are recorded by Super SID system during February, March, and April, 2013. Then VLF data were compared with the GOES satellite data found in the Space Environment Center online database. The main factors of the variation in VLF signal intensities recorded by the Super SID system are class, duration of the solar flare and the frequency of VLF signals.
dc.identifier.doi10.3103/S1541308X16030079
dc.identifier.endpage237
dc.identifier.issn1541-308X
dc.identifier.issn1934-807X
dc.identifier.issue3
dc.identifier.orcid0000-0002-4504-5750
dc.identifier.scopus2-s2.0-85009732683
dc.identifier.scopusqualityQ3
dc.identifier.startpage232
dc.identifier.urihttps://doi.org/10.3103/S1541308X16030079
dc.identifier.urihttps://hdl.handle.net/11508/52546
dc.identifier.volume24
dc.identifier.wosWOS:000393038800007
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAllerton Press Inc
dc.relation.ispartofPhysics of Wave Phenomena
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260511
dc.subjectIhy
dc.titleThe effects of solar flares on the very low frequency signals recorded by super SID system
dc.typeArticle

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