Solar Active Region Magnetogram Image Dataset for Studies of Space Weather
Not on the map. Why?
Abstract (arXiv)
In this dataset we provide a comprehensive collection of magnetograms (images quantifying the strength of the magnetic field) from the National Aeronautics and Space Administration's (NASA's) Solar Dynamics Observatory (SDO). The dataset incorporates data from three sources and provides SDO Helioseismic and Magnetic Imager (HMI) magnetograms of solar active regions (regions of large magnetic flux, generally the source of eruptive events) as well as labels of corresponding flaring activity. This dataset will be useful for image analysis or solar physics research related to magnetic structure, its evolution over time, and its relation to solar flares. The dataset will be of interest to those researchers investigating automated solar flare prediction methods, including supervised and unsupervised machine learning (classical and deep), binary and multi-class classification, and regression. This dataset is a minimally processed, user configurable dataset of consistently sized images of solar active regions that can serve as a benchmark dataset for solar flare prediction research.
Key facts. Cited by 1 paper in the map (data through 14 Oct 2026). Builds on 6 of its 60 references that are in the map. First posted on arXiv 16 May 2023.
Builds on
6 of 60 references.
References · 6
- 2015Deep Residual Learning for Image Recognitioncited by 52,096
- 2014Very Deep Convolutional Networks for Large-Scale Image Recognitioncited by 15,364
- 2015Rethinking the Inception Architecture for Computer Visioncited by 5,475
- 2019Predicting Solar Flares Using a Long Short-Term Memory Networkcited by 25
- 2022Predicting Solar Flares Using CNN and LSTM on Two Solar Cycles of Active Region Datacited by 15
- 2020A Framework for Designing and Evaluating Solar Flare Forecasting Systemscited by 4
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Citing papers per year: 2025: 1.
1 paper.