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dc.contributor.authorTank, SB
dc.contributor.authorTuncer, MK
dc.contributor.authorMalin, Stuart R.C.
dc.contributor.authorYazıcı-Çakın, Oya
dc.contributor.authorOzcan, O
dc.date.accessioned2021-03-04T09:27:21Z
dc.date.available2021-03-04T09:27:21Z
dc.date.issued2000
dc.identifier.citationMalin S. R. , Ozcan O., Tank S., Tuncer M., Yazıcı-Çakın O., "Geomagnetic signature of the 1999 August 11 total eclipse", GEOPHYSICAL JOURNAL INTERNATIONAL, cilt.140, sa.3, 2000
dc.identifier.issn0956-540X
dc.identifier.otherav_684e5310-0a3d-4ef0-8b5c-fc4371626d3b
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/72309
dc.identifier.urihttps://doi.org/10.1046/j.1365-246x.2000.00061.x
dc.description.abstractThe magnetic north (H), magnetic east (D) and vertically downward (Z) components of the geomagnetic field were monitored at Elazig, Turkey, with a three-component fluxgate magnetometer during the 1999 August 11 total eclipse of the Sun. The results were compared with those obtained with an identical instrument at Kandilli magnetic observatory, which is at a similar latitude to Elazig, but clear of the band of totality. An increase of D is found during the eclipse, rising to a maximum close to the time of maximum eclipse. The reality of this effect is confirmed by noting a similar feature, also centred on the time of eclipse, at a number of European observatories.
dc.language.isoeng
dc.subjectYerbilimleri
dc.subjectMühendislik ve Teknoloji
dc.subjectJeofizik Mühendisliği
dc.subjectTemel Bilimler (SCI)
dc.subjectJEOKİMYA VE JEOFİZİK
dc.titleGeomagnetic signature of the 1999 August 11 total eclipse
dc.typeMakale
dc.relation.journalGEOPHYSICAL JOURNAL INTERNATIONAL
dc.contributor.department, ,
dc.identifier.volume140
dc.identifier.issue3
dc.contributor.firstauthorID727583


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