Image Details
Caption: Figure 18.
Performance of the Kelvin–Helmholtz flux corrector network is compared over time compared to the uncorrected network on a test set. While the network was only trained until t = 1.0 (∼1000 time steps), we find significant improvement over the baseline until t ∼ 3.0, which is far into the nonlinear regime.
© 2026. The Author(s). Published by the American Astronomical Society.