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arxiv_ml 85% Match Research Paper Planetary Scientists,Astrophysicists,Climate Modelers,Machine Learning Researchers,Computational Scientists 4 days ago

Accelerating Radiative Transfer for Planetary Atmospheres by Orders of Magnitude with a Transformer-Based Machine Learning Model

generative-ai › autoregressive
📄 Abstract

Abstract: Radiative transfer calculations are essential for modeling planetary atmospheres. However, standard methods are computationally demanding and impose accuracy-speed trade-offs. High computational costs force numerical simplifications in large models (e.g., General Circulation Models) that degrade the accuracy of the simulation. Radiative transfer calculations are an ideal candidate for machine learning emulation: fundamentally, it is a well-defined physical mapping from a static atmospheric profile to the resulting fluxes, and high-fidelity training data can be created from first principles calculations. We developed a radiative transfer emulator using an encoder-only transformer neural network architecture, trained on 1D profiles representative of solar-composition hot Jupiter atmospheres. Our emulator reproduced bolometric two-stream layer fluxes with mean test set errors of ~1% compared to the traditional method and achieved speedups of 100x. Emulating radiative transfer with machine learning opens up the possibility for faster and more accurate routines within planetary atmospheric models such as GCMs.
Authors (4)
Isaac Malsky
Tiffany Kataria
Natasha E. Batalha
Matthew Graham
Submitted
October 30, 2025
arXiv Category
astro-ph.EP
arXiv PDF

Key Contributions

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.

Business Value

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.