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The ionospheric slab thickness (τ) is an important parameter for studying the dynamic of the ionosphere. The slab thickness is often determined by a combination technique of Global Navigation Satellite System (GNSS) and ionosonde. However, this technique is not optimal due to the sparsely p...

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Main Author: KASYFU AMBARA (NIM : 15110045 ) ; Pembimbing I : Dr. techn. Dudy D. Wijaya, S.T., M.Sc. ; Pem, AUZAN
Format: Final Project
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/18114
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Institution: Institut Teknologi Bandung
Language: Indonesia
id id-itb.:18114
spelling id-itb.:181142017-10-09T10:51:12Z#TITLE_ALTERNATIVE# KASYFU AMBARA (NIM : 15110045 ) ; Pembimbing I : Dr. techn. Dudy D. Wijaya, S.T., M.Sc. ; Pem, AUZAN Indonesia Final Project INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/18114 The ionospheric slab thickness (τ) is an important parameter for studying the dynamic of the ionosphere. The slab thickness is often determined by a combination technique of Global Navigation Satellite System (GNSS) and ionosonde. However, this technique is not optimal due to the sparsely populated of ionosonde stations in Indonesia. The purposes of this research is to optimize the use of single GNSS receiver to determine the ionospheric slab thickness without receiving any help from other techniques, to validate the results with a combination technique of Global Navigation Satellite System (GNSS) and ionosonde, and to study its physical characteristics. The method which is used in this research is a new approach from the improvement of geometric-free formula called Improved Geometric Free (IGF). The IGF formula is then applied to determine the slab thickness in 2011 and 2012 by using IGS (International GNSS Service) station data which is managed by BIG (Geospatial Information Agency). The validation results obtained correlation values between the two methods in 2011 and 2012 were 0.64 and 0.60, and the RMS deviations were 155.51 km and 210.19 km. The category correlation concluded that the ionospheric slab thickness which is obtained from the single GNSS receiver is relevant to be applied for ionospheric slab thickness (τ) study. Finally, by analyzing the data of the ionospheric slab thickness in 2011 and 2012, the physical characteristics of daily, seasonal, and correlation with the physical characteristics of the sunspot number could be acquired. text
institution Institut Teknologi Bandung
building Institut Teknologi Bandung Library
continent Asia
country Indonesia
Indonesia
content_provider Institut Teknologi Bandung
collection Digital ITB
language Indonesia
description The ionospheric slab thickness (τ) is an important parameter for studying the dynamic of the ionosphere. The slab thickness is often determined by a combination technique of Global Navigation Satellite System (GNSS) and ionosonde. However, this technique is not optimal due to the sparsely populated of ionosonde stations in Indonesia. The purposes of this research is to optimize the use of single GNSS receiver to determine the ionospheric slab thickness without receiving any help from other techniques, to validate the results with a combination technique of Global Navigation Satellite System (GNSS) and ionosonde, and to study its physical characteristics. The method which is used in this research is a new approach from the improvement of geometric-free formula called Improved Geometric Free (IGF). The IGF formula is then applied to determine the slab thickness in 2011 and 2012 by using IGS (International GNSS Service) station data which is managed by BIG (Geospatial Information Agency). The validation results obtained correlation values between the two methods in 2011 and 2012 were 0.64 and 0.60, and the RMS deviations were 155.51 km and 210.19 km. The category correlation concluded that the ionospheric slab thickness which is obtained from the single GNSS receiver is relevant to be applied for ionospheric slab thickness (τ) study. Finally, by analyzing the data of the ionospheric slab thickness in 2011 and 2012, the physical characteristics of daily, seasonal, and correlation with the physical characteristics of the sunspot number could be acquired.
format Final Project
author KASYFU AMBARA (NIM : 15110045 ) ; Pembimbing I : Dr. techn. Dudy D. Wijaya, S.T., M.Sc. ; Pem, AUZAN
spellingShingle KASYFU AMBARA (NIM : 15110045 ) ; Pembimbing I : Dr. techn. Dudy D. Wijaya, S.T., M.Sc. ; Pem, AUZAN
#TITLE_ALTERNATIVE#
author_facet KASYFU AMBARA (NIM : 15110045 ) ; Pembimbing I : Dr. techn. Dudy D. Wijaya, S.T., M.Sc. ; Pem, AUZAN
author_sort KASYFU AMBARA (NIM : 15110045 ) ; Pembimbing I : Dr. techn. Dudy D. Wijaya, S.T., M.Sc. ; Pem, AUZAN
title #TITLE_ALTERNATIVE#
title_short #TITLE_ALTERNATIVE#
title_full #TITLE_ALTERNATIVE#
title_fullStr #TITLE_ALTERNATIVE#
title_full_unstemmed #TITLE_ALTERNATIVE#
title_sort #title_alternative#
url https://digilib.itb.ac.id/gdl/view/18114
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