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Develops a transformer-based machine learning model that emulates radiative transfer calculations for planetary atmospheres, achieving speedups of 100x with mean test set errors of ~1% compared to traditional methods. This significantly reduces computational costs, enabling more accurate and detailed simulations in large-scale models like General Circulation Models.
Enables faster and more accurate climate and atmospheric simulations for planets, leading to better understanding of exoplanet atmospheres and potentially improving Earth's climate models. This can accelerate scientific discovery and inform climate policy.