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Given the same trajectory data from a p=3 simulation of the backward facing step, we are observing differences in GNN model convergence between recent Aurora and older Polaris runs, with the Polaris runs reaching deeper convergence. The difference is apparent after a few thousand training iterations.
Given the same trajectory data from a p=3 simulation of the backward facing step, we are observing differences in GNN model convergence between recent Aurora and older Polaris runs, with the Polaris runs reaching deeper convergence. The difference is apparent after a few thousand training iterations.
GNN model parameters used:
Things to check:
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