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nasa-ibm-ai4science/ar_segmentation_surya
ar_segmentation_surya is a machine learning model from nasa-ibm-ai4science. Use it for the machine learning task on the model card, and read the license before you ship it in a product. The card lists the license as apache-2.0.
This repository hosts fine-tuned weights of Surya – a heliophysics foundation model – for the task of solar Active Region (AR) segmentation. Solar Active Regions are magnetically complex structures associated with fla…
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Updated Aug 20, 2025
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From the Hugging Face model README
This repository hosts fine-tuned weights of Surya – a heliophysics foundation model – for the task of solar Active Region (AR) segmentation.
Solar Active Regions are magnetically complex structures associated with flares and coronal mass ejections (CMEs). Within ARs, the Polarity Inversion Line (PIL) serves as a critical precursor of eruptions. Accurate segmentation of ARs containing PILs is essential for space weather forecasting and understanding solar magnetic complexity.
We benchmarked Surya against a standard UNet baseline on the ARPIL dataset.
| Model | Params | IoU | Dice Coeff |
|---|---|---|---|
| UNet | 9.2 M | 0.688 | 0.801 |
| Surya (LoRA) | 4.1 M | 0.768 | 0.853 |
Surya achieves higher segmentation quality with fewer parameters, highlighting the benefits of foundation model pretraining and parameter-efficient adaptation.
Follow the instructions at Surya/downstream_examples/ar_segmentation