Please use this identifier to cite or link to this item: https://ptsldigital.ukm.my/jspui/handle/123456789/784398
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dc.contributor.authorSiti Aminah Bahari-
dc.contributor.authorMardina Abdullah-
dc.contributor.authorBaharudin Yatim-
dc.contributor.editorMahamod Ismail-
dc.date.accessioned2026-08-11T07:19:01Z-
dc.date.available2026-08-11T07:19:01Z-
dc.identifier.isbn978-1-4244-4956-9en_US
dc.identifier.urihttps://ptsldigital.ukm.my/jspui/handle/123456789/784398-
dc.description.abstractWe have studied the variations of TEC at quasiconjugate points using data obtained from GPS receiver at Sew station Antarctica (SYOG) (GC 49.99 5, 39.38 E COM MMS, 7L65 E's and Arbolt station (ARIO), Iceland 15 period in 2007, during the minimum phase of Big Artic region) (GC 66.19 N. 34289 E: CGM: 6437S ryck 23. The GPS measurements of IGS and IMO network we used to create 12 maps The time resolution of TEC about 1 hour. The TEC maps show that the maximum TEC value ever SVOG is at 1000 LT (1300 LT) while in ARHO i NUT (UT-LT) March 2007, when it was summer in the polar region, the TEC valer aver SYOG ramp was Apher by 3 TECU than ARHO, which was experiencing winter dering that time. This has proved the rule af sun in the TEC but with photoionization process. The measurements of the TEC variation obtained from GPS during different months at both hemispheres showed symmetry in the median TEC at the conjugate points.en_US
dc.language.isoenen_US
dc.subjectConjugate pointsen_US
dc.subjectTECen_US
dc.subjectGeomagnetic stormsen_US
dc.titleVariations of ionospheric TEC at geomagnetic conjugate points during solar minimumen_US
dc.typeSeminar Papersen_US
dc.format.pages157-160en_US
dc.identifier.callnoQB495.I557 2009 semen_US
dc.contributor.conferencenameInternational Conference on Space Science & Communication (IconSpace)-
dc.coverage.conferencelocationThistle Port Dickson Resort, Negeri Sembilan-
dc.date.conferencedate2009-10-26-
Appears in Collections:Seminar Papers/ Proceedings / Kertas Kerja Seminar/ Prosiding

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