Auroral breakup detection in all-sky images by unsupervised learning

Due to a large number of automatic auroral camera systems on the ground, image data analysis requires more efficiency than what human expert visual inspection can provide. Furthermore, there is no solid consensus on how many different types or shapes exist in auroral displays. We report the first at...

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Main Authors: Partamies, Noora, Dol, Bas, Teissier, Vincent, Juusola, Liisa, Syrjäsuo, Mikko, Mulders, Hjalmar
Format: Text
Language:English
Published: 2024
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2023-2857
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2857/
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spelling ftcopernicus:oai:publications.copernicus.org:egusphere116342 2024-09-15T18:38:27+00:00 Auroral breakup detection in all-sky images by unsupervised learning Partamies, Noora Dol, Bas Teissier, Vincent Juusola, Liisa Syrjäsuo, Mikko Mulders, Hjalmar 2024-04-25 application/pdf https://doi.org/10.5194/egusphere-2023-2857 https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2857/ eng eng doi:10.5194/egusphere-2023-2857 https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2857/ eISSN: Text 2024 ftcopernicus https://doi.org/10.5194/egusphere-2023-2857 2024-08-28T05:24:15Z Due to a large number of automatic auroral camera systems on the ground, image data analysis requires more efficiency than what human expert visual inspection can provide. Furthermore, there is no solid consensus on how many different types or shapes exist in auroral displays. We report the first attempt to classify auroral morphological forms by an unsupervised learning method on an image set that contains both nightside and dayside aurora. We used 6 months of full-colour auroral all-sky images captured at a high-Arctic observatory on Svalbard, Norway, in 2019–2020. The selection of images containing aurora was performed manually. These images were then input into a convolutional neural network called SimCLR for feature extraction. The clustered and fused features resulted in 37 auroral morphological clusters. In the clustering of auroral image data with two different time resolutions, we found that the occurrence of 8 clusters strongly increased when the image cadence was high (24 s), while the occurrence of 14 clusters experienced little or no change with changes in input image cadence. We therefore investigated the temporal evolution of a group of eight “active aurora” clusters. Time periods for which this active aurora persisted for longer than two consecutive images with a maximum cadence of 6 min coincided with ground-magnetic deflections, and their occurrence was found to maximize around magnetic midnight. The active aurora onsets typically included vortical auroral structures and equivalent current patterns typical for substorms. Our findings therefore suggest that our unsupervised image clustering method can be used to detect auroral breakups in ground-based image datasets with a temporal accuracy determined by the image cadence. Text Svalbard Copernicus Publications: E-Journals
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Due to a large number of automatic auroral camera systems on the ground, image data analysis requires more efficiency than what human expert visual inspection can provide. Furthermore, there is no solid consensus on how many different types or shapes exist in auroral displays. We report the first attempt to classify auroral morphological forms by an unsupervised learning method on an image set that contains both nightside and dayside aurora. We used 6 months of full-colour auroral all-sky images captured at a high-Arctic observatory on Svalbard, Norway, in 2019–2020. The selection of images containing aurora was performed manually. These images were then input into a convolutional neural network called SimCLR for feature extraction. The clustered and fused features resulted in 37 auroral morphological clusters. In the clustering of auroral image data with two different time resolutions, we found that the occurrence of 8 clusters strongly increased when the image cadence was high (24 s), while the occurrence of 14 clusters experienced little or no change with changes in input image cadence. We therefore investigated the temporal evolution of a group of eight “active aurora” clusters. Time periods for which this active aurora persisted for longer than two consecutive images with a maximum cadence of 6 min coincided with ground-magnetic deflections, and their occurrence was found to maximize around magnetic midnight. The active aurora onsets typically included vortical auroral structures and equivalent current patterns typical for substorms. Our findings therefore suggest that our unsupervised image clustering method can be used to detect auroral breakups in ground-based image datasets with a temporal accuracy determined by the image cadence.
format Text
author Partamies, Noora
Dol, Bas
Teissier, Vincent
Juusola, Liisa
Syrjäsuo, Mikko
Mulders, Hjalmar
spellingShingle Partamies, Noora
Dol, Bas
Teissier, Vincent
Juusola, Liisa
Syrjäsuo, Mikko
Mulders, Hjalmar
Auroral breakup detection in all-sky images by unsupervised learning
author_facet Partamies, Noora
Dol, Bas
Teissier, Vincent
Juusola, Liisa
Syrjäsuo, Mikko
Mulders, Hjalmar
author_sort Partamies, Noora
title Auroral breakup detection in all-sky images by unsupervised learning
title_short Auroral breakup detection in all-sky images by unsupervised learning
title_full Auroral breakup detection in all-sky images by unsupervised learning
title_fullStr Auroral breakup detection in all-sky images by unsupervised learning
title_full_unstemmed Auroral breakup detection in all-sky images by unsupervised learning
title_sort auroral breakup detection in all-sky images by unsupervised learning
publishDate 2024
url https://doi.org/10.5194/egusphere-2023-2857
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2857/
genre Svalbard
genre_facet Svalbard
op_source eISSN:
op_relation doi:10.5194/egusphere-2023-2857
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2857/
op_doi https://doi.org/10.5194/egusphere-2023-2857
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