The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines

Scintillation caused by the electron density irregularities in the ionospheric plasma leads to rapid fluctuations in the amplitude and phase of the Global Navigation Satellite Systems (GNSS) signals. Ionospheric scintillation severely degrades the performance of the GNSS receiver in the signal acqui...

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Published in:Sensors
Main Authors: Caner Savas, Fabio Dovis
Format: Text
Language:English
Published: Multidisciplinary Digital Publishing Institute 2019
Subjects:
Online Access:https://doi.org/10.3390/s19235219
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spelling ftmdpi:oai:mdpi.com:/1424-8220/19/23/5219/ 2023-08-20T04:01:54+02:00 The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines Caner Savas Fabio Dovis 2019-11-28 application/pdf https://doi.org/10.3390/s19235219 EN eng Multidisciplinary Digital Publishing Institute Physical Sensors https://dx.doi.org/10.3390/s19235219 https://creativecommons.org/licenses/by/4.0/ Sensors; Volume 19; Issue 23; Pages: 5219 GNSS scintillation support vector machines kernel Gaussian polynomial Text 2019 ftmdpi https://doi.org/10.3390/s19235219 2023-07-31T22:50:23Z Scintillation caused by the electron density irregularities in the ionospheric plasma leads to rapid fluctuations in the amplitude and phase of the Global Navigation Satellite Systems (GNSS) signals. Ionospheric scintillation severely degrades the performance of the GNSS receiver in the signal acquisition, tracking, and positioning. By utilizing the GNSS signals, detecting and monitoring the scintillation effects to decrease the effect of the disturbing signals have gained importance, and machine learning-based algorithms have been started to be applied for the detection. In this paper, the performance of Support Vector Machines (SVM) for scintillation detection is discussed. The effect of the different kernel functions, namely, linear, Gaussian, and polynomial, on the performance of the SVM algorithm is analyzed. Performance is statistically assessed in terms of probabilities of detection and false alarm of the scintillation event. Real GNSS signals that are affected by significant phase and amplitude scintillation effect, collected at the South African Antarctic research base SANAE IV and Hanoi, Vietnam have been used in this study. This paper questions how to select a suitable kernel function by analyzing the data preparation, cross-validation, and experimental test stages of the SVM-based process for scintillation detection. It has been observed that the overall accuracy of fine Gaussian SVM outperforms the linear, which has the lowest complexity and running time. Moreover, the third-order polynomial kernel provides improved performance compared to linear, coarse, and medium Gaussian kernel SVMs, but it comes with a cost of increased complexity and running time. Text Antarc* Antarctic MDPI Open Access Publishing Antarctic Base SANAE IV ENVELOPE(-2.850,-2.850,-71.667,-71.667) SANAE ENVELOPE(-2.850,-2.850,-71.667,-71.667) SANAE IV ENVELOPE(-2.850,-2.850,-71.667,-71.667) Sensors 19 23 5219
institution Open Polar
collection MDPI Open Access Publishing
op_collection_id ftmdpi
language English
topic GNSS
scintillation
support vector machines
kernel
Gaussian
polynomial
spellingShingle GNSS
scintillation
support vector machines
kernel
Gaussian
polynomial
Caner Savas
Fabio Dovis
The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines
topic_facet GNSS
scintillation
support vector machines
kernel
Gaussian
polynomial
description Scintillation caused by the electron density irregularities in the ionospheric plasma leads to rapid fluctuations in the amplitude and phase of the Global Navigation Satellite Systems (GNSS) signals. Ionospheric scintillation severely degrades the performance of the GNSS receiver in the signal acquisition, tracking, and positioning. By utilizing the GNSS signals, detecting and monitoring the scintillation effects to decrease the effect of the disturbing signals have gained importance, and machine learning-based algorithms have been started to be applied for the detection. In this paper, the performance of Support Vector Machines (SVM) for scintillation detection is discussed. The effect of the different kernel functions, namely, linear, Gaussian, and polynomial, on the performance of the SVM algorithm is analyzed. Performance is statistically assessed in terms of probabilities of detection and false alarm of the scintillation event. Real GNSS signals that are affected by significant phase and amplitude scintillation effect, collected at the South African Antarctic research base SANAE IV and Hanoi, Vietnam have been used in this study. This paper questions how to select a suitable kernel function by analyzing the data preparation, cross-validation, and experimental test stages of the SVM-based process for scintillation detection. It has been observed that the overall accuracy of fine Gaussian SVM outperforms the linear, which has the lowest complexity and running time. Moreover, the third-order polynomial kernel provides improved performance compared to linear, coarse, and medium Gaussian kernel SVMs, but it comes with a cost of increased complexity and running time.
format Text
author Caner Savas
Fabio Dovis
author_facet Caner Savas
Fabio Dovis
author_sort Caner Savas
title The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines
title_short The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines
title_full The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines
title_fullStr The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines
title_full_unstemmed The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines
title_sort impact of different kernel functions on the performance of scintillation detection based on support vector machines
publisher Multidisciplinary Digital Publishing Institute
publishDate 2019
url https://doi.org/10.3390/s19235219
long_lat ENVELOPE(-2.850,-2.850,-71.667,-71.667)
ENVELOPE(-2.850,-2.850,-71.667,-71.667)
ENVELOPE(-2.850,-2.850,-71.667,-71.667)
geographic Antarctic
Base SANAE IV
SANAE
SANAE IV
geographic_facet Antarctic
Base SANAE IV
SANAE
SANAE IV
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source Sensors; Volume 19; Issue 23; Pages: 5219
op_relation Physical Sensors
https://dx.doi.org/10.3390/s19235219
op_rights https://creativecommons.org/licenses/by/4.0/
op_doi https://doi.org/10.3390/s19235219
container_title Sensors
container_volume 19
container_issue 23
container_start_page 5219
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