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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ftpubmed:oai:pubmedcentral.nih.gov:6928998 2023-05-15T13:43:29+02:00 The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines † Savas, Caner Dovis, Fabio 2019-11-28 http://www.ncbi.nlm.nih.gov/pmc/articles/PMC6928998/ http://www.ncbi.nlm.nih.gov/pubmed/31795093 https://doi.org/10.3390/s19235219 en eng MDPI http://www.ncbi.nlm.nih.gov/pmc/articles/PMC6928998/ http://www.ncbi.nlm.nih.gov/pubmed/31795093 http://dx.doi.org/10.3390/s19235219 © 2019 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/). CC-BY Article Text 2019 ftpubmed https://doi.org/10.3390/s19235219 2019-12-29T01:31:40Z 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 PubMed Central (PMC) 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 |
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Article Savas, Caner Dovis, Fabio The Impact of Different Kernel Functions on the Performance of Scintillation Detection Based on Support Vector Machines † |
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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 |
Savas, Caner Dovis, Fabio |
author_facet |
Savas, Caner Dovis, Fabio |
author_sort |
Savas, Caner |
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 |
MDPI |
publishDate |
2019 |
url |
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC6928998/ http://www.ncbi.nlm.nih.gov/pubmed/31795093 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_relation |
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC6928998/ http://www.ncbi.nlm.nih.gov/pubmed/31795093 http://dx.doi.org/10.3390/s19235219 |
op_rights |
© 2019 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/). |
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CC-BY |
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https://doi.org/10.3390/s19235219 |
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