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  5. Doppler and pseudorange measurements as prediction features for multi-constellation GNSS LoS/NLoS signal classification

Doppler and pseudorange measurements as prediction features for multi-constellation GNSS LoS/NLoS signal classification

Publication date
2023-08-28
Document type
Konferenzbeitrag
Author
Zidan, Jasmine
Anyaegbu, Esther
Kampert, Erik  
Higgins, Matthew D.
Ford, Colin
Organisational unit
Grundlagen der Elektrotechnik  
DOI
10.1109/swc57546.2023.10449004
URI
https://openhsu.ub.hsu-hh.de/handle/10.24405/22750
Conference
20th IEEE Autonomous and Trusted Vehicles Conference (ATC 2023) ; Portsmouth, United Kingdom ; August 28–31, 2023
Publisher
IEEE
Book title
2023 IEEE Smart World Congress (SWC)
ISBN
979-8-3503-1980-4
Peer-reviewed
✅
Part of the university bibliography
✅
Additional Information
Language
English
Abstract
Precise positioning and timing are key challenges for safety security critical applications in autonomous and trusted vehicles (ATVs). A global navigation satellite system (GNSS) receiver is one of the sensors used in ATVs to provide a satellite-based positioning, navigation and timing solution. GNSS robustness in built-up areas like urban canyons and in sheltered locations like multi-storey car parks is severely impaired due to non-line-of-sight and multi-path signal propagation. In this paper, an optimised decision tree classifier is used for the discrimination of GNSS signals into line-of-sight and non-line-of-sight signals. In addition to using the carrier-to-noise ratio and the satellite elevation angle as prediction features, adding the pseudoranges and the Doppler measurements enhances the classifier performance by 12 %. As a result, an overall prediction accuracy of 97.8 % is obtained. For the studied data-set, the pseudorange measurements have a higher prediction importance than the Doppler measurements. Also evaluated in this study, is the use of a GPS L1 signal prediction regression model on other GNSS constellations. Analysis of the investigated scenario shows that the use of the current model is not adequate for non-GPS constellations.
Version
Published version
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