Please use this identifier to cite or link to this item: https://ptsldigital.ukm.my/jspui/handle/123456789/784396
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dc.contributor.authorRiri Darwanisari Didong-
dc.contributor.authorMohammad Awad Momani-
dc.contributor.editorMahamod Ismail-
dc.date.accessioned2026-08-11T06:58:22Z-
dc.date.available2026-08-11T06:58:22Z-
dc.identifier.isbn978-1-4244-4956-9en_US
dc.identifier.urihttps://ptsldigital.ukm.my/jspui/handle/123456789/784396-
dc.description.abstractThe paper examines the ionspheric responses to the annular solar eclipse on 26 January 2009 over Southern Atlantic, Australia and Indian Ocean. The solar eclipse event took place during quiet solar and magnetic activities with maximum Kp and Dst indices are 3 and -32 nT. The external contacts of penumbra U1 and U4 occurred at 06:02:39 UT in the South Atlantic and 09:54:44 UT in the Celebes Sea. The GPS Total Electron Content (TEC) measurements obtained from 5 GPS stations belonging to International GNSS Service (IGS) network over India, Australia, and Antarctica have been employed in the analysis. 5 stations had been selected to conduct this study. They are Syowa in Antarctica, Windhoek in Namibia, Indian Institute of Science in India, Ceduna and Kerguelen Islands in Australia. The observations showed clear depletion in the TEC level from about 0.4 to 20% during the eclipse period.en_US
dc.language.isoenen_US
dc.subjectSolar eclipseen_US
dc.subjectGPSen_US
dc.subjectIonosphereen_US
dc.subjectTECen_US
dc.titleThe ionospheric response to the annular solar eclipse on 26th January 2009en_US
dc.typeSeminar Papersen_US
dc.format.pages147-152en_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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