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Developing Machine Learning Models of Subgrid Turbulent Transport for Quiet-Sun 3D Radiative Hydrodynamic Simulations

  • Authors: Rimsha Hameed Syeda, Dustin Kempton, Viacheslav Sadykov, Irina Kitiashvili, Rafal Angryk

Rimsha Hameed Syeda et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 11.

Frequency plots of the deviations of τvv in panel (a) and τuw in panel (b) between the predictions of the best CNN model (purple), Smagorinsky CS = CC = 0.001 (green), and gradient models (red) and the target value.

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