Auroral breakup detection in all-sky images by unsupervised learning

IF 1.7 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Annales Geophysicae Pub Date : 2023-11-30 DOI:10.5194/egusphere-2023-2857
Noora Partamies, Bas Dol, Vincent Teissier, Liisa Juusola, Mikko Syrjäsuo, Hjalmar Mulders
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Abstract

Abstract. Due to a large number of automatic auroral camera systems on the ground, the image data analysis requires more efficiency than what a 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 unsupervised learning method on an image set that contains both nightside and dayside aurora. We used six 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 to a convolutional neural network called SimCLR for feature extraction. The clustered and fused features resulted in 37 auroral morphological classes. In the classification of auroral image data with two different time resolutions we found that the occurrence of eight morphological classes strongly increased when the image cadence was high (24 seconds), while the occurrence of 13 morphological classes experienced little or no change with changes in input image cadence. We therefore investigated the temporal evolution of the group of eight "active auroral classes". Time periods for which "active auroral classes" persisted for longer than two consecutive images with maximum cadence of six minutes coincided with ground-magnetic deflections and their occurrence was found clustered around the magnetic midnight. The active auroral onsets typically included vortical auroral structures and equivalent current patterns typical for substorms. Our findings therefore suggest that our unsupervised image classification method can be used to detect auroral breakups in ground-based image datasets with a temporal accuracy determined by the image cadence.
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基于无监督学习的全天图像极光破碎检测
摘要。由于地面上有大量的自动极光相机系统,因此图像数据分析需要比人类专家视觉检查提供的效率更高。此外,关于极光有多少种不同的类型或形状,目前还没有明确的共识。我们报告了第一次尝试用无监督学习方法对包含夜侧和日侧极光的图像集进行极光形态分类。我们使用了2019-2020年在挪威斯瓦尔巴群岛的高纬度观测站拍摄的六个月的全彩极光全天图像。选择包含极光的图像是手动执行的。然后将这些图像输入到一个名为SimCLR的卷积神经网络中进行特征提取。聚类和融合的特征产生了37个极光形态分类。在两种不同时间分辨率的极光图像数据分类中,我们发现,当图像节奏高(24秒)时,8种形态类别的出现率明显增加,而13种形态类别的出现率随着输入图像节奏的变化而变化不大或没有变化。因此,我们研究了8个“活跃极光类”的时间演化。“活跃极光群”持续时间超过连续两幅图像且最大间隔为6分钟的时间段与地磁偏转相吻合,并且它们的出现被发现集中在磁性午夜附近。活跃的极光发作通常包括涡旋极光结构和亚暴典型的等效电流模式。因此,我们的研究结果表明,我们的无监督图像分类方法可以用于检测地面图像数据集中的极光分裂,其时间精度由图像节奏决定。
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来源期刊
Annales Geophysicae
Annales Geophysicae 地学-地球科学综合
CiteScore
4.30
自引率
0.00%
发文量
42
审稿时长
2 months
期刊介绍: Annales Geophysicae (ANGEO) is a not-for-profit international multi- and inter-disciplinary scientific open-access journal in the field of solar–terrestrial and planetary sciences. ANGEO publishes original articles and short communications (letters) on research of the Sun–Earth system, including the science of space weather, solar–terrestrial plasma physics, the Earth''s ionosphere and atmosphere, the magnetosphere, and the study of planets and planetary systems, the interaction between the different spheres of a planet, and the interaction across the planetary system. Topics range from space weathering, planetary magnetic field, and planetary interior and surface dynamics to the formation and evolution of planetary systems.
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