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license: apache-2.0
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---
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license: apache-2.0
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language:
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- en
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base_model:
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- nasa-ibm-ai4science/Surya-1.0
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---
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# π Surya β Active Region Segmentation
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## π Model Overview
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This repository hosts **fine-tuned weights of Surya** β a heliophysics foundation model β for the task of **solar Active Region (AR) segmentation**.
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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.
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---
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## π Results
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We benchmarked Surya against a standard UNet baseline on the ARPIL dataset.
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| Model | Params | IoU | Dice Coeff |
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|--------|--------|-------|------------|
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| UNet | 9.2 M | 0.688 | 0.801 |
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| **Surya (LoRA)** | **4.1 M** | **0.768** | **0.853** |
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Surya achieves **higher segmentation quality with fewer parameters**, highlighting the benefits of foundation model pretraining and parameter-efficient adaptation.
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---
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## πΌ Example
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<p align="center">
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<img src="figure/ar_seg_results.png" width="100%">
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</p>
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- **Top Row**: Input SDO/HMI data (Date: 2014-02-01, Time: 08:12)
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- **Middle Row**: Surya segmentation output
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- **Bottom Row**: Ground Truth
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---
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## β‘ Usage
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Follow the instructions at [Surya/downstream_examples/ar_segmentation](https://github.com/NASA-IMPACT/Surya/tree/main/downstream_examples/ar_segmentation)
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---
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## π€ Acknowledgements
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- **NASA IMPACT** and **IBM** for developing the Surya foundation model
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