Please use this identifier to cite or link to this item: https://ptsldigital.ukm.my/jspui/handle/123456789/784395
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dc.contributor.authorMohammad Awad Momani-
dc.contributor.editorMahamod Ismail-
dc.date.accessioned2026-08-11T06:56:16Z-
dc.date.available2026-08-11T06:56:16Z-
dc.identifier.isbn978-1-4244-4956-9en_US
dc.identifier.urihttps://ptsldigital.ukm.my/jspui/handle/123456789/784395-
dc.description.abstracthe ionospheric response to the 1st August 2008 total solar eclipse has been investigated at three incoherent scatter radar stations over Europe and Greenland (e.g. Svalbard, Tromso and Sondrestrom). The observations electron density, decrease in show obvious temperature, ion velocity and plasma cutoff frequency during the period of solar eclipse particularly between 09:00 and 10:00 UT. The depletion was clearly seen in the E and F1 layers at altitudes below 200 km where in these regions the depletion was synchronous with the eclipse function. In the F2 layer of ionosphere (300-400 km), different response was seen with long period of electron density reduction and reduction in F2 maximum occurred between 10:00 and 15:00 UT. A comparison between the electron and ion temperature response at Tromso station shows a significant decrease in electron temperature only (value of -700 K).en_US
dc.language.isoenen_US
dc.subjectIonosphereen_US
dc.subjectRadaren_US
dc.subjectSolar eclipseen_US
dc.titleThe ionospheric response to the 1st August 2008 total solar eclipse using incoherent scatter radar measurementsen_US
dc.typeSeminar Papersen_US
dc.format.pages142-146en_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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