A dataset of manually annotated filaments from H-alpha observations

We present the Manually Annotated GONG Filaments in H-alpha Observations (MAGFiLO v1.0) dataset. This dataset contains 10,244 annotated filaments from 1,593 observations captured by the Global Oscillation Network Group (GONG), spanning the years 2011 through 2022. Each annotation details one filament's segmentation, minimum bounding box, spine, and magnetic field chirality. With a total of over one thousand person-hours of annotation, and a double-blind review process, we ensured high-quality ground-truth data. Our inter-annotator agreement reaches a Kappa score of 0.66. We also verified that the hemispheric preference of filaments as annotated in MAGFiLO aligns with the findings from similar datasets of much smaller sample sizes. MAGFiLO is the first dataset of its size, enabling advanced deep learning models to identify filaments and their features with unprecedented precision. It also provides a testbed for solar physicists interested in large-scale analysis of filaments. In this report, we document the details of the annotation and the post-processing phases that were applied.

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Publication Details

Journal
Scientific Data
Published
2024-09-27
DOI
https://doi.org/10.1038/s41597-024-03876-y
Citations
4
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
2.64

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A dataset of manually annotated filaments from H-alpha observations

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4 citations
Scientific Data
Astrophysics and Cosmic Phenomena
2.64
article

A dataset of manually annotated filaments from H-alpha observations

Samuel Alan McDonald, Dustin Kempton, Azim Ahmadzadeh, Eugene Yu‐Chuan Kang, P. C. H. Martens, Luca Bertello, Alexei Pevtsov, V. Aparna, Alexander Pevtsov, Sri Harsha Seelamneni, Laxmi Alekhya Nagubandi, Aya Abdelkarem, Rohan Adhyapak, Kartik Chaurasiya, Apaar Bawa, N. L. DOUGLAS, Riley Wu, Patrick M Copeland
article en
4 citations

Abstract

We present the Manually Annotated GONG Filaments in H-alpha Observations (MAGFiLO v1.0) dataset. This dataset contains 10,244 annotated filaments from 1,593 observations captured by the Global Oscillation Network Group (GONG), spanning the years 2011 through 2022. Each annotation details one filament's segmentation, minimum bounding box, spine, and magnetic field chirality. With a total of over one thousand person-hours of annotation, and a double-blind review process, we ensured high-quality ground-truth data. Our inter-annotator agreement reaches a Kappa score of 0.66. We also verified that the hemispheric preference of filaments as annotated in MAGFiLO aligns with the findings from similar datasets of much smaller sample sizes. MAGFiLO is the first dataset of its size, enabling advanced deep learning models to identify filaments and their features with unprecedented precision. It also provides a testbed for solar physicists interested in large-scale analysis of filaments. In this report, we document the details of the annotation and the post-processing phases that were applied.

Scientific DataVol. 11(1)
Georgia Institute of Technology (US), Kennesaw State University (US), Georgia State University (US), University of Missouri–St. Louis (US), National Solar Observatory (US), Oaks Hospital (GB), Bay Area Environmental Research Institute (US)
National Science Foundation, Instituto de Astrofísica de Canarias, Directorate for Computer and Information Science and Engineering, National Oceanic and Atmospheric Administration, Office of Advanced Cyberinfrastructure
Zero hunger
Openalex Percentile: Top 7%
Astrophysics and Cosmic Phenomena
2.64
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