A generated image can become a request to a solar archive: find an observed magnetic region with a similar configuration. A 2026 study demonstrates that sequence by linking an image generator to physically meaningful controls and an image-retrieval model.[1]
The real observations come from Space-weather HMI Active Region Patches, or SHARPs, derived from NASA’s Solar Dynamics Observatory. Each patch tracks a concentration of magnetic activity through its visible lifetime, with measurements every 12 minutes. Alongside magnetic-field maps, the original SHARP pipeline calculates quantities including total magnetic flux and spatial field gradients. It therefore provides both a pattern to examine and numerical descriptions of the magnetic region.[2]
Turning a property into a query
The authors trained on 49,552 maps from 1,839 distinct patches observed between May 2010 and July 2023. A generative adversarial network creates images. Support-vector machines identify directions in its internal coordinates that change summed field strength or separation between magnetic polarities. A third model retrieves similar archive images.[1]
For 1,000 generated queries, the unsigned-field sums of queries and retrieved observations had a Pearson correlation of 0.78; polarity separation correlated at 0.28. Here, 1 would mean a perfect positive linear relationship. Some physical properties therefore matched more closely than others. Exact calibration of the controls to physical units remains future work.[1]
The result gives researchers a route from a hypothetical magnetic configuration to a real observation they can investigate.[1]
Sources & further reading
- Deep Generative model that uses physical quantities to generate and retrieve solar magnetic active regions arXiv; accepted author manuscript for The Astrophysical Journal Supplement Series · 20 Feb 2026 · Accessed 20 Oct 2026
- The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches Solar Physics · 30 Apr 2014 · Accessed 20 Oct 2026