Automatic Identification of Aurora Fold Structure in All-Sky Images

Identification of small-scale auroral structures is key to searching for auroral events. However, it is impracticable for humans to manually select sufficient aurora events for statistical analysis, and it is also challenging for computers because of the non-rigid shape and fluid nature of auroras....

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Published in:Universe
Main Authors: Qian Wang, Haonan Fang, Bin Li
Format: Article in Journal/Newspaper
Language:English
Published: MDPI AG 2023
Subjects:
Online Access:https://doi.org/10.3390/universe9020079
https://doaj.org/article/2e25533422ac4d03a4b06be68c92e67f
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spelling ftdoajarticles:oai:doaj.org/article:2e25533422ac4d03a4b06be68c92e67f 2023-05-15T17:48:28+02:00 Automatic Identification of Aurora Fold Structure in All-Sky Images Qian Wang Haonan Fang Bin Li 2023-02-01T00:00:00Z https://doi.org/10.3390/universe9020079 https://doaj.org/article/2e25533422ac4d03a4b06be68c92e67f EN eng MDPI AG https://www.mdpi.com/2218-1997/9/2/79 https://doaj.org/toc/2218-1997 doi:10.3390/universe9020079 2218-1997 https://doaj.org/article/2e25533422ac4d03a4b06be68c92e67f Universe, Vol 9, Iss 79, p 79 (2023) aurora all-sky image aurora fold structure small-scale structure skeleton extraction automatic identification Elementary particle physics QC793-793.5 article 2023 ftdoajarticles https://doi.org/10.3390/universe9020079 2023-02-26T01:28:04Z Identification of small-scale auroral structures is key to searching for auroral events. However, it is impracticable for humans to manually select sufficient aurora events for statistical analysis, and it is also challenging for computers because of the non-rigid shape and fluid nature of auroras. Fold structure is the most common type of auroral small-scale structure, and its appearance is indicative of a variety of auroral events. This paper proposes a small-scale aurora structure identification framework to automatically detect aurora fold structures. First, the location and shape of auroras are identified based on a deep learning segmentation network. Then, the skeleton of the auroral shape is extracted to represent the trajectories of auroras. Finally, the proposed skeleton-based fold identification module (SFIM) can detect the aurora fold structure. To evaluate the effectiveness of the proposed method, we built an aurora fold structure sample dataset, namely F-dataset, containing 2000 images at 557.7 nm obtained by the all-sky imagers at Yellow River Station (YRS), Ny-Ålesund, Svalbard. Experimental results show that automatic identification can achieve good consistency with human perception. Statistical analysis of over 30,000 images shows that the fold occurrence has a distinct double-peak distribution at pre-noon and post-noon. Article in Journal/Newspaper Ny Ålesund Ny-Ålesund Svalbard Directory of Open Access Journals: DOAJ Articles Ny-Ålesund Svalbard Universe 9 2 79
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic aurora
all-sky image
aurora fold structure
small-scale structure
skeleton extraction
automatic identification
Elementary particle physics
QC793-793.5
spellingShingle aurora
all-sky image
aurora fold structure
small-scale structure
skeleton extraction
automatic identification
Elementary particle physics
QC793-793.5
Qian Wang
Haonan Fang
Bin Li
Automatic Identification of Aurora Fold Structure in All-Sky Images
topic_facet aurora
all-sky image
aurora fold structure
small-scale structure
skeleton extraction
automatic identification
Elementary particle physics
QC793-793.5
description Identification of small-scale auroral structures is key to searching for auroral events. However, it is impracticable for humans to manually select sufficient aurora events for statistical analysis, and it is also challenging for computers because of the non-rigid shape and fluid nature of auroras. Fold structure is the most common type of auroral small-scale structure, and its appearance is indicative of a variety of auroral events. This paper proposes a small-scale aurora structure identification framework to automatically detect aurora fold structures. First, the location and shape of auroras are identified based on a deep learning segmentation network. Then, the skeleton of the auroral shape is extracted to represent the trajectories of auroras. Finally, the proposed skeleton-based fold identification module (SFIM) can detect the aurora fold structure. To evaluate the effectiveness of the proposed method, we built an aurora fold structure sample dataset, namely F-dataset, containing 2000 images at 557.7 nm obtained by the all-sky imagers at Yellow River Station (YRS), Ny-Ålesund, Svalbard. Experimental results show that automatic identification can achieve good consistency with human perception. Statistical analysis of over 30,000 images shows that the fold occurrence has a distinct double-peak distribution at pre-noon and post-noon.
format Article in Journal/Newspaper
author Qian Wang
Haonan Fang
Bin Li
author_facet Qian Wang
Haonan Fang
Bin Li
author_sort Qian Wang
title Automatic Identification of Aurora Fold Structure in All-Sky Images
title_short Automatic Identification of Aurora Fold Structure in All-Sky Images
title_full Automatic Identification of Aurora Fold Structure in All-Sky Images
title_fullStr Automatic Identification of Aurora Fold Structure in All-Sky Images
title_full_unstemmed Automatic Identification of Aurora Fold Structure in All-Sky Images
title_sort automatic identification of aurora fold structure in all-sky images
publisher MDPI AG
publishDate 2023
url https://doi.org/10.3390/universe9020079
https://doaj.org/article/2e25533422ac4d03a4b06be68c92e67f
geographic Ny-Ålesund
Svalbard
geographic_facet Ny-Ålesund
Svalbard
genre Ny Ålesund
Ny-Ålesund
Svalbard
genre_facet Ny Ålesund
Ny-Ålesund
Svalbard
op_source Universe, Vol 9, Iss 79, p 79 (2023)
op_relation https://www.mdpi.com/2218-1997/9/2/79
https://doaj.org/toc/2218-1997
doi:10.3390/universe9020079
2218-1997
https://doaj.org/article/2e25533422ac4d03a4b06be68c92e67f
op_doi https://doi.org/10.3390/universe9020079
container_title Universe
container_volume 9
container_issue 2
container_start_page 79
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