Please use this identifier to cite or link to this item: http://dspace.unimap.edu.my:80/xmlui/handle/123456789/8613
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dc.contributor.authorAbdull Zubi, Ahmad-
dc.contributor.authorAhmad Faizal, Mohd Zain-
dc.date.accessioned2010-08-12T04:03:48Z-
dc.date.available2010-08-12T04:03:48Z-
dc.date.issued2009-06-20-
dc.identifier.citationp.1-5en_US
dc.identifier.urihttp://dspace.unimap.edu.my/123456789/8613-
dc.descriptionMUCEET 2009 is organized by Malaysian Technical Universities Network (MTUN) comprising of Universiti Malaysia Perlis (UniMAP), Universiti Tun Hussein Onn (UTHM), Universiti Teknikal Melaka (UTeM) and Universiti Malaysia Pahang (UMP), 20th - 22nd June 2009 at M. S. Garden Hotel, Kuantan, Pahang.en_US
dc.description.abstractThe measurements of ionospheric drift and convection using the digital doppler interferometer at the Wireless and Radio Science centre (Waras) at UTHM, is used to provide high temporal and spatial resolution measurements of the dynamics of the ionosphere at the Parit Raja station in Batu Pahat, Johor. These measurements include Doppler shifts, angles of arrival, as well as group ranges from the significant numbers of ionospheric echo sources simultaneously at the same time. By employing Doppler inteferometry reception technique at four receivers connected to four spaced antennas nearby, it is possible to identify the three dimensional locations of various scattering points reflected back from the ionosphere as a result of vertically-incident HF waves transmitted at frequencies of 5.9MHz, 7MHz, and 8MHz. These three frequencies cover the local F-layers since the critical frequencies lie between 6MHz and 8MHz for this local station. The technique of Doppler interferometry treats signal returns from the ionospheric F-region as reflections from individual scatterers. Spectral analysis is performed on the complex voltages generated from the four receivers’ in-phase (I) and quadrature-phase (Q) detectors to produce Doppler frequency functions. Both spectral phase functions and amplitude functions are generated using Fast Fourier Transform or FFT by the receivers from the Doppler frequency functions. This will then result in a skymap display containing echo coordinates, ranges and Doppler shifts. By further processing of the echoes, drift velocities which can be deduced by a least-squares fitting algorithm can be found. The behaviour of the plasma movements under certain variations of the geomagnetic and solar activities can also be studied so as to be able to estimate the influence of geomagnetic storms and equatorial electrojets on the ionosphere, which is vital for navigation, surveillance and telecommunications.en_US
dc.language.isoenen_US
dc.publisherUniversiti Malaysia Pahang (UMP)en_US
dc.relation.ispartofseriesProceedings of the Malaysian Technical Universities Conference on Engineering and Technology (MUCEET) 2009en_US
dc.subjectDoppler driften_US
dc.subjectDoppler interferometryen_US
dc.subjectIonosphereen_US
dc.subjectSkymapen_US
dc.subjectSpaced antennasen_US
dc.subjectMalaysian Technical Universities Conference on Engineering and Technology (MUCEET)en_US
dc.titleEquatorial F-region plasma drift measurements and observations using Doppler interferometry at Parit Rajaen_US
dc.typeWorking Paperen_US
Appears in Collections:Conference Papers

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