Solar Active Region Magnetogram Image Dataset for Studies of Space Weather
arXiv:2305.09492 · doi:10.1038/s41597-023-02628-8
Abstract
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.
References in corpus (17)
- The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs -- Space-weather HMI Active Region Patches
- Solar Flare Prediction Using SDO/HMI Vector Magnetic Field Data with a Machine-Learning Algorithm
- Predicting Solar Flares Using a Long Short-Term Memory Network
- Predicting Solar Flares Using SDO/HMI Vector Magnetic Data Product and Random Forest Algorithm
- Predicting Solar Flares Using CNN and LSTM on Two Solar Cycles of Active Region Data
- Predicting solar flares with machine learning: investigating solar cycle dependence
- Prediction of Solar Flares Using Unique Signatures of Magnetic Field Images
- Operational solar flare prediction model using Deep Flare Net
- An automated classification approach to ranking photospheric proxies of magnetic energy build-up
- The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Magnetohydrodynamics Simulation Module for the Global Solar Corona
- Evaluating (and Improving) Estimates of the Solar Radial Magnetic Field Component from Line-of-Sight Magnetograms
- Fine-grained Solar Flare Forecasting Based on the Hybrid Convolutional Neural Networks
- Supervised convolutional neural networks for classification of flaring and nonflaring active regions using line-of-sight magnetograms
- Decreasing False Alarm Rates in ML-based Solar Flare Prediction using SDO/HMI Data
- A Framework for Designing and Evaluating Solar Flare Forecasting Systems
- Machine Learning Approaches to Solar-Flare Forecasting: Is Complex Better?
- Solar Active Region Magnetogram Image Dataset for Studies of Space Weather
Cited by in corpus (4)
- Solar Active Region Magnetogram Image Dataset for Studies of Space Weather
- Solar Flare Prediction Using Long Short-term Memory (LSTM) and Decomposition-LSTM with Sliding Window Pattern Recognition
- Solar flare forecasting with foundational transformer models across image, video, and time-series modalities
- Bypassing the static input size of neural networks in flare forecasting by using spatial pyramid pooling