Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias

Magnetic Data Acquisition System (MAGDAS) through its Circum-Pan Pacific Magnetometer Network (CPMN) is a real time system magnetometers. The ordinary data from the MAGDAS is one of the datar that can be used for research or studies of variations like magnetic storm and aurora sub storms. The earth...

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Bibliographic Details
Main Author:	Alias, Omar Mokhtar
Format:	Thesis
Language:	English
Published:	2013
Subjects:	Theoretical astronomy and celestial mechanics Geomagnetism
Online Access:	https://ir.uitm.edu.my/id/eprint/68356/1/68356.pdf
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id	my-uitm-ir.68356
record_format	uketd_dc
spelling	my-uitm-ir.683562023-07-21T02:46:23Z Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias 2013 Alias, Omar Mokhtar Theoretical astronomy and celestial mechanics Geomagnetism Magnetic Data Acquisition System (MAGDAS) through its Circum-Pan Pacific Magnetometer Network (CPMN) is a real time system magnetometers. The ordinary data from the MAGDAS is one of the datar that can be used for research or studies of variations like magnetic storm and aurora sub storms. The earth magnetic data that obtain from MAGDAS can also be used as earth magnetic data observation for space events such as geomagnetic storm. Geomagnetic storms one of the event that can damage satellites disable electric power grids. This paper focuses on monitoring and analysis MAGDAS data during the occurrence of space events such as geomagnetic storms and during ionosphere events such as Travelling Ionospheric Disturbance (TID) at different stations. The raw data is taken from different MAGDAS unit which are supplied by the Space Environment Research Centre (SERC) Kyushu University, Japan. The data were taken at different station to see its characterization and the different of earth magnetic field. Matlab program is used to simulate the MAGDAS data. Kp index also used as reference to identified the variations of ionosphere events. The results has been studies and analysis has been made. Result shown that there are 3 phase of geomagnetic storm occurrence. Through the earth magnetic field horizontal intensity (parameter H), TID have been detect. TID happen during occurrence of the aurora. 2013 Thesis https://ir.uitm.edu.my/id/eprint/68356/ https://ir.uitm.edu.my/id/eprint/68356/1/68356.pdf text en public degree Universiti Teknologi MARA (UiTM) Faculty of Electrical Engineering Ya'acob, Norsuzila
institution	Universiti Teknologi MARA
collection	UiTM Institutional Repository
language	English
advisor	Ya'acob, Norsuzila
topic	Theoretical astronomy and celestial mechanics Geomagnetism
spellingShingle	Theoretical astronomy and celestial mechanics Geomagnetism Alias, Omar Mokhtar Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias
description	Magnetic Data Acquisition System (MAGDAS) through its Circum-Pan Pacific Magnetometer Network (CPMN) is a real time system magnetometers. The ordinary data from the MAGDAS is one of the datar that can be used for research or studies of variations like magnetic storm and aurora sub storms. The earth magnetic data that obtain from MAGDAS can also be used as earth magnetic data observation for space events such as geomagnetic storm. Geomagnetic storms one of the event that can damage satellites disable electric power grids. This paper focuses on monitoring and analysis MAGDAS data during the occurrence of space events such as geomagnetic storms and during ionosphere events such as Travelling Ionospheric Disturbance (TID) at different stations. The raw data is taken from different MAGDAS unit which are supplied by the Space Environment Research Centre (SERC) Kyushu University, Japan. The data were taken at different station to see its characterization and the different of earth magnetic field. Matlab program is used to simulate the MAGDAS data. Kp index also used as reference to identified the variations of ionosphere events. The results has been studies and analysis has been made. Result shown that there are 3 phase of geomagnetic storm occurrence. Through the earth magnetic field horizontal intensity (parameter H), TID have been detect. TID happen during occurrence of the aurora.
format	Thesis
qualification_level	Bachelor degree
author	Alias, Omar Mokhtar
author_facet	Alias, Omar Mokhtar
author_sort	Alias, Omar Mokhtar
title	Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias
title_short	Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias
title_full	Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias
title_fullStr	Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias
title_full_unstemmed	Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias
title_sort	travelling ionospgeric disturbance (tid) during the occurrence of geomagnetic storm using magdas data / omar mokhtar alias
granting_institution	Universiti Teknologi MARA (UiTM)
granting_department	Faculty of Electrical Engineering
publishDate	2013
url	https://ir.uitm.edu.my/id/eprint/68356/1/68356.pdf
_version_	1783735772390621184

Travelling ionospgeric disturbance (TID) during the occurrence of geomagnetic storm using MAGDAS data / Omar Mokhtar Alias

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