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A Deep Generative Model that Uses Physical Quantities to Generate and Retrieve Solar Magnetic Active Regions

  • Authors: Subhamoy Chatterjee, Andrés Muñoz-Jaramillo, Anna Malanushenko

Subhamoy Chatterjee et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 6.

Result of GAN approximation (bottom row) of real images (top row) as a function of AR center heliocentric angle (﹩{\cos }^{-1}\mu ﹩). The two-dimensional histogram in the right panel shows that the reconstruction loss (i.e., the mean squared error between real and GAN-approximated images) increase when the AR moves toward the solar limb.

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