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Paper · arXiv

MAGiDiff: Sampling the Photospheric Vector Field from UV/EUV Filtergrams

Photospheric vector magnetic fields are foundational to modeling, understanding, and forecasting solar activity. These data are usually produced by inverting and disambiguating the full Stokes vector at multiple passbands, which is demanding. Here, we investigate how well we can estimate photospheric vector magnetograms from UV/EUV filtergrams. This problem is challenging and intrinsically ambiguous without polarization information, as the mapping from UV/EUV intensity to the magnetic field is indirect and ill-posed. We introduce MAGiDiff, a machine-learning-based method that uses denoising diffusion models to estimate vector magnetograms from UV/EUV filtergrams. As input, MAGiDiff takes ...

AuthorsRuoyu Wang, David Fouhey
Primary categoryastro-ph.SR
Published30 September 2026
Last updated at source30 September 2026
astro-ph.SRastro-ph.IMcs.CV
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