mlsanityData to 14 Oct 2026

Super-Resolution of Solar Magnetograms via Adaptive Stratified Ensemble Learning with Uncertainty Estimation

arXiv 2609.27131 ↗First posted 22 Sep 2026cs.CV astro-ph.SRcited by 0

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Abstract (arXiv)

Single-image super-resolution of Sun's photospheric magnetograms enables consistent analysis across heterogeneous space-based instruments and supports long-term studies of solar magnetic field evolution. We address the super-resolution task from SOHO/MDI (low-resolution) to SDO/HMI (high-resolution) line-of-sight (LOS) magnetograms using a modified RRDBNet architecture initialized by ESRGAN pretrained weights. Through systematic per-image diagnostic analysis, we identify image complexity as the dominant predictor of reconstruction errors. To exploit this finding, we introduce an adaptive stratified specialist ensemble (SSE) of three specialist networks with uncertainty estimation, where each specialist network is trained by images from three different complexity strata using a weighted random sampling strategy. During inference, a lightweight router based on input image statistics assigns each test image to the appropriate specialist network. Our experimental results demonstrate the good performance of the proposed ensemble and its superiority over closely related methods.

Key facts. No citing papers in the map yet (data through 14 Oct 2026). Builds on 12 of its 25 references that are in the map. First posted on arXiv 22 Sep 2026.

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12 of 25 references.

References · 12

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  6. 2020Better Aggregation in Test-Time Augmentationcited by 122
  7. 2024Pixel-level and Semantic-level Adjustable Super-resolution: A Dual-LoRA Approachcited by 97
  8. 2021Balanced-MixUp for Highly Imbalanced Medical Image Classificationcited by 46
  9. 2025Uncertainty-guided Perturbation for Image Super-Resolution Diffusion Modelcited by 29
  10. 2017Enhancing SDO/HMI images using deep learningcited by 11
  11. 2019Progressive Perception-Oriented Network for Single Image Super-Resolutioncited by 7
  12. 2022A Deep Learning Approach to Generating Photospheric Vector Magnetograms of Solar Active Regions for SOHO/MDI Using SDO/HMI and BBSO Datacited by 5

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