Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 12.

The scatter plots of two components: τvv in panel (a) and τuw in panel (b), comparing the predictions of the best CNN model and the gradient model. Blue points show the predictions of CNN, and red points show the predictions of the gradient model.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse