LEO satellite clock analysis and prediction for positioning applications

The positioning service aided by low Earth orbit (LEO) mega-constellations has become a hot topic in recent years. To achieve precise positioning, accuracy of the LEO clocks is important for single-receiver users. To bridge the gap between the applicable time of the clock products and the time of po...

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Main Authors: Kan Wang, Ahmed El-Mowafy
Format: Article
Language:English
Published: Taylor & Francis Group 2021-06-01
Series:Geo-spatial Information Science
Subjects:
leo
uso
Online Access:http://dx.doi.org/10.1080/10095020.2021.1917310
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spelling doaj-55c3117e622c4fce81bdda1d29f292bd2021-06-11T09:33:06ZengTaylor & Francis GroupGeo-spatial Information Science1009-50201993-51532021-06-010012010.1080/10095020.2021.19173101917310LEO satellite clock analysis and prediction for positioning applicationsKan Wang0Ahmed El-Mowafy1Curtin UniversityCurtin UniversityThe positioning service aided by low Earth orbit (LEO) mega-constellations has become a hot topic in recent years. To achieve precise positioning, accuracy of the LEO clocks is important for single-receiver users. To bridge the gap between the applicable time of the clock products and the time of positioning, the precise LEO clocks need to be predicted over a certain period depending on the sampling interval of the clock products. This study discusses the prediction errors for periods from 10 s to 1 h for two typical LEO clock types, i.e. the ultra-stable oscillator (USO) and the oven-controlled crystal oscillator (OCXO). The prediction is based on GNSS-determined precise clock estimates, where the clock stability is related to the GNSS estimation errors, the behaviors of the oscillators themselves, the systematic effects related to the environment and the relativistic effects, and the stability of the time reference. Based on real data analysis, LEO clocks of the two different types are simulated under different conditions, and a prediction model considering the systematic effects is proposed. Compared to a simple polynomial fitting model usually applied, the proposed model can significantly reduce the prediction errors, i.e. by about 40%-70% in simulations and about 5%-30% for real data containing different miss-modeled effects. For both clock types, short-term prediction of 1 min would result in a root mean square error (RMSE) of a few centimeters when using a very stable time reference. The RMSE amounts to about 0.1 m, when a typical real-time time reference of the national center for space studies (CNES) real-time clocks was used. For long-term prediction of 1 h, the RMSE could range from below 1 m to a few meters for the USOs, depending on the complexity of the miss-modeled effects. For OCXOs, the 1 h prediction could lead to larger errors with an RMSE of about 10 m.http://dx.doi.org/10.1080/10095020.2021.1917310leoclock predictionusoocxorelativistic effects
collection DOAJ
language English
format Article
sources DOAJ
author Kan Wang
Ahmed El-Mowafy
spellingShingle Kan Wang
Ahmed El-Mowafy
LEO satellite clock analysis and prediction for positioning applications
Geo-spatial Information Science
leo
clock prediction
uso
ocxo
relativistic effects
author_facet Kan Wang
Ahmed El-Mowafy
author_sort Kan Wang
title LEO satellite clock analysis and prediction for positioning applications
title_short LEO satellite clock analysis and prediction for positioning applications
title_full LEO satellite clock analysis and prediction for positioning applications
title_fullStr LEO satellite clock analysis and prediction for positioning applications
title_full_unstemmed LEO satellite clock analysis and prediction for positioning applications
title_sort leo satellite clock analysis and prediction for positioning applications
publisher Taylor & Francis Group
series Geo-spatial Information Science
issn 1009-5020
1993-5153
publishDate 2021-06-01
description The positioning service aided by low Earth orbit (LEO) mega-constellations has become a hot topic in recent years. To achieve precise positioning, accuracy of the LEO clocks is important for single-receiver users. To bridge the gap between the applicable time of the clock products and the time of positioning, the precise LEO clocks need to be predicted over a certain period depending on the sampling interval of the clock products. This study discusses the prediction errors for periods from 10 s to 1 h for two typical LEO clock types, i.e. the ultra-stable oscillator (USO) and the oven-controlled crystal oscillator (OCXO). The prediction is based on GNSS-determined precise clock estimates, where the clock stability is related to the GNSS estimation errors, the behaviors of the oscillators themselves, the systematic effects related to the environment and the relativistic effects, and the stability of the time reference. Based on real data analysis, LEO clocks of the two different types are simulated under different conditions, and a prediction model considering the systematic effects is proposed. Compared to a simple polynomial fitting model usually applied, the proposed model can significantly reduce the prediction errors, i.e. by about 40%-70% in simulations and about 5%-30% for real data containing different miss-modeled effects. For both clock types, short-term prediction of 1 min would result in a root mean square error (RMSE) of a few centimeters when using a very stable time reference. The RMSE amounts to about 0.1 m, when a typical real-time time reference of the national center for space studies (CNES) real-time clocks was used. For long-term prediction of 1 h, the RMSE could range from below 1 m to a few meters for the USOs, depending on the complexity of the miss-modeled effects. For OCXOs, the 1 h prediction could lead to larger errors with an RMSE of about 10 m.
topic leo
clock prediction
uso
ocxo
relativistic effects
url http://dx.doi.org/10.1080/10095020.2021.1917310
work_keys_str_mv AT kanwang leosatelliteclockanalysisandpredictionforpositioningapplications
AT ahmedelmowafy leosatelliteclockanalysisandpredictionforpositioningapplications
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