Whistler Waves Detection - Investigation of modern machine learning techniques to detect and characterise whistler waves

Lightning strokes create powerful electromagnetic pulses that routinely cause very low frequency (VLF) waves to propagate across hemispheres along geomagnetic field lines. VLF antenna receivers can be used to detect these whistler waves generated by these lightning strokes. The particular time/frequ...

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Bibliographic Details
Main Author: Konan, Othniel Jean Ebenezer Yao
Other Authors: Mishra, Amit, Lotz, Stefan
Format: Master Thesis
Language:English
Published: Faculty of Engineering and the Built Environment 2021
Subjects:
Online Access:http://hdl.handle.net/11427/35746
https://open.uct.ac.za/bitstream/11427/35746/1/thesis_ebe_2021_konan%20othniel%20jean%20ebenezer%20yao.pdf
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spelling ftunivcapetownir:oai:localhost:11427/35746 2023-05-15T13:32:17+02:00 Whistler Waves Detection - Investigation of modern machine learning techniques to detect and characterise whistler waves Konan, Othniel Jean Ebenezer Yao Mishra, Amit Lotz, Stefan 2021_ application/pdf http://hdl.handle.net/11427/35746 https://open.uct.ac.za/bitstream/11427/35746/1/thesis_ebe_2021_konan%20othniel%20jean%20ebenezer%20yao.pdf eng eng Faculty of Engineering and the Built Environment Department of Electrical Engineering http://hdl.handle.net/11427/35746 https://open.uct.ac.za/bitstream/11427/35746/1/thesis_ebe_2021_konan%20othniel%20jean%20ebenezer%20yao.pdf Very Low Frequency Waves Whistler Radio Waves CFAR Object detection Master Thesis Masters MSc 2021 ftunivcapetownir 2022-09-13T05:52:36Z Lightning strokes create powerful electromagnetic pulses that routinely cause very low frequency (VLF) waves to propagate across hemispheres along geomagnetic field lines. VLF antenna receivers can be used to detect these whistler waves generated by these lightning strokes. The particular time/frequency dependence of the received whistler wave enables the estimation of electron density in the plasmasphere region of the magnetosphere. Therefore the identification and characterisation of whistlers are important tasks to monitor the plasmasphere in real time and to build large databases of events to be used for statistical studies. The current state of the art in detecting whistler is the Automatic Whistler Detection (AWD) method developed by Lichtenberger (2009) [1]. This method is based on image correlation in 2 dimensions and requires significant computing hardware situated at the VLF receiver antennas (e.g. in Antarctica). The aim of this work is to develop a machine learning based model capable of automatically detecting whistlers in the data provided by the VLF receivers. The approach is to use a combination of image classification and localisation on the spectrogram data generated by the VLF receivers to identify and localise each whistler. The data at hand has around 2300 events identified by AWD at SANAE and Marion and will be used as training, validation, and testing data. Three detector designs have been proposed. The first one using a similar method to AWD, the second using image classification on regions of interest extracted from a spectrogram, and the last one using YOLO, the current state of the art in object detection. It has been shown that these detectors can achieve a misdetection and false alarm rate, respectively, of less than 15% on Marion's dataset. It is important to note that the ground truth (initial whistler label) for data used in this study was generated using AWD. Moreover, SANAE IV data was small and did not provide much content in the study. Master Thesis Antarc* Antarctica University of Cape Town: OpenUCT SANAE ENVELOPE(-2.850,-2.850,-71.667,-71.667) SANAE IV ENVELOPE(-2.850,-2.850,-71.667,-71.667)
institution Open Polar
collection University of Cape Town: OpenUCT
op_collection_id ftunivcapetownir
language English
topic Very Low Frequency Waves
Whistler Radio Waves
CFAR
Object detection
spellingShingle Very Low Frequency Waves
Whistler Radio Waves
CFAR
Object detection
Konan, Othniel Jean Ebenezer Yao
Whistler Waves Detection - Investigation of modern machine learning techniques to detect and characterise whistler waves
topic_facet Very Low Frequency Waves
Whistler Radio Waves
CFAR
Object detection
description Lightning strokes create powerful electromagnetic pulses that routinely cause very low frequency (VLF) waves to propagate across hemispheres along geomagnetic field lines. VLF antenna receivers can be used to detect these whistler waves generated by these lightning strokes. The particular time/frequency dependence of the received whistler wave enables the estimation of electron density in the plasmasphere region of the magnetosphere. Therefore the identification and characterisation of whistlers are important tasks to monitor the plasmasphere in real time and to build large databases of events to be used for statistical studies. The current state of the art in detecting whistler is the Automatic Whistler Detection (AWD) method developed by Lichtenberger (2009) [1]. This method is based on image correlation in 2 dimensions and requires significant computing hardware situated at the VLF receiver antennas (e.g. in Antarctica). The aim of this work is to develop a machine learning based model capable of automatically detecting whistlers in the data provided by the VLF receivers. The approach is to use a combination of image classification and localisation on the spectrogram data generated by the VLF receivers to identify and localise each whistler. The data at hand has around 2300 events identified by AWD at SANAE and Marion and will be used as training, validation, and testing data. Three detector designs have been proposed. The first one using a similar method to AWD, the second using image classification on regions of interest extracted from a spectrogram, and the last one using YOLO, the current state of the art in object detection. It has been shown that these detectors can achieve a misdetection and false alarm rate, respectively, of less than 15% on Marion's dataset. It is important to note that the ground truth (initial whistler label) for data used in this study was generated using AWD. Moreover, SANAE IV data was small and did not provide much content in the study.
author2 Mishra, Amit
Lotz, Stefan
format Master Thesis
author Konan, Othniel Jean Ebenezer Yao
author_facet Konan, Othniel Jean Ebenezer Yao
author_sort Konan, Othniel Jean Ebenezer Yao
title Whistler Waves Detection - Investigation of modern machine learning techniques to detect and characterise whistler waves
title_short Whistler Waves Detection - Investigation of modern machine learning techniques to detect and characterise whistler waves
title_full Whistler Waves Detection - Investigation of modern machine learning techniques to detect and characterise whistler waves
title_fullStr Whistler Waves Detection - Investigation of modern machine learning techniques to detect and characterise whistler waves
title_full_unstemmed Whistler Waves Detection - Investigation of modern machine learning techniques to detect and characterise whistler waves
title_sort whistler waves detection - investigation of modern machine learning techniques to detect and characterise whistler waves
publisher Faculty of Engineering and the Built Environment
publishDate 2021
url http://hdl.handle.net/11427/35746
https://open.uct.ac.za/bitstream/11427/35746/1/thesis_ebe_2021_konan%20othniel%20jean%20ebenezer%20yao.pdf
long_lat ENVELOPE(-2.850,-2.850,-71.667,-71.667)
ENVELOPE(-2.850,-2.850,-71.667,-71.667)
geographic SANAE
SANAE IV
geographic_facet SANAE
SANAE IV
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation http://hdl.handle.net/11427/35746
https://open.uct.ac.za/bitstream/11427/35746/1/thesis_ebe_2021_konan%20othniel%20jean%20ebenezer%20yao.pdf
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