The CHASM-SWPC Dataset for Coronal Hole Detection & Analysis

• URL: http://arxiv.org/abs/2511.14044v1
• Date: Tue, 18 Nov 2025 01:51:13 GMT
• Title: The CHASM-SWPC Dataset for Coronal Hole Detection & Analysis
• Abstract summary: Coronal holes (CHs) are low-activity, low-density solar coronal regions with open magnetic field lines.<n>We developed a semi-automated pipeline to digitize SWPC maps into binary segmentation masks.<n>The resulting masks constitute the CHASM-SWPC dataset to train and test automated CH detection models.
• Score: 2.0515802800471485
• License: http://creativecommons.org/licenses/by-nc-sa/4.0/
• Abstract: Coronal holes (CHs) are low-activity, low-density solar coronal regions with open magnetic field lines (Cranmer 2009). In the extreme ultraviolet (EUV) spectrum, CHs appear as dark patches. Using daily hand-drawn maps from the Space Weather Prediction Center (SWPC), we developed a semi-automated pipeline to digitize the SWPC maps into binary segmentation masks. The resulting masks constitute the CHASM-SWPC dataset, a high-quality dataset to train and test automated CH detection models, which is released with this paper. We developed CHASM (Coronal Hole Annotation using Semi-automatic Methods), a software tool for semi-automatic annotation that enables users to rapidly and accurately annotate SWPC maps. The CHASM tool enabled us to annotate 1,111 CH masks, comprising the CHASM-SWPC-1111 dataset. We then trained multiple CHRONNOS (Coronal Hole RecOgnition Neural Network Over multi-Spectral-data) architecture (Jarolim et al. 2021) neural networks using the CHASM-SWPC dataset and compared their performance. Training the CHRONNOS neural network on these data achieved an accuracy of 0.9805, a True Skill Statistic (TSS) of 0.6807, and an intersection-over-union (IoU) of 0.5668, which is higher than the original pretrained CHRONNOS model Jarolim et al. (2021) achieved an accuracy of 0.9708, a TSS of 0.6749, and an IoU of 0.4805, when evaluated on the CHASM-SWPC-1111 test set.

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