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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 18.

The scatter plots of two components τvv in panel (a) and τuw in panel (b), comparing the predictions of the 3DCNN1 trained with data before and after normalization. Blue dots represent the predictions of CNN when trained with normalized data, and green represents the predictions of CNN when trained without a log transform.

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