Interpretable Neural Networks to Predict Momentum Fluxes of Orographic Gravity Waves

Fuente: arXiv
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Autori principali: Haslauer, Elias, Schwabe, Mierk, Dörnbrack, Andreas, Gerber, Edwin P., Rapp, Markus, Žagar, Nedjeljka, Eyring, Veronika
Natura: Preprint
Pubblicazione: 2026
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author Haslauer, Elias
Schwabe, Mierk
Dörnbrack, Andreas
Gerber, Edwin P.
Rapp, Markus
Žagar, Nedjeljka
Eyring, Veronika
author_facet Haslauer, Elias
Schwabe, Mierk
Dörnbrack, Andreas
Gerber, Edwin P.
Rapp, Markus
Žagar, Nedjeljka
Eyring, Veronika
contents State-of-the-art Earth system models (ESMs) cannot explicitly resolve many small-scale atmospheric processes such as atmospheric gravity waves, and thus must represent, or parameterise, their effects on the resolved state. Machine learning (ML) has the potential to improve these parameterisations. In our study, we train neural networks (NNs) on ERA5 reanalysis data to predict momentum fluxes of orographic gravity waves as a function of the state variables at the resolution of a coarse ESM. Employing a full year of data, we extract inertia-gravity waves using the software MODES, which applies linear theory for wave filtering, and train ML models on data coarse-grained to the ESM's target resolution. We consider four different cases: the full spectrum of inertia-gravity waves resolved in ERA5, or just the part of the spectrum that is subgrid-scale in the target ESM, both over all land or just over mountainous terrain. Our NNs successfully predict momentum fluxes, with a global coefficient of determination ($R^2$) ranging from 0.72 to 0.56, depending on the case, when evaluated offline with data from another year. An analysis of our models using SHAP values, an explainable AI technique, suggests that the networks learned physically meaningful relationships. In addition, we give a comparison with the physics-based parameterisation scheme by Lott and Miller. This work forms the basis for the development of operational ML-based parameterisations to improve the representation of gravity waves and their effects in climate models.
format Preprint
id arxiv_https___arxiv_org_abs_2605_05052
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Interpretable Neural Networks to Predict Momentum Fluxes of Orographic Gravity Waves
Haslauer, Elias
Schwabe, Mierk
Dörnbrack, Andreas
Gerber, Edwin P.
Rapp, Markus
Žagar, Nedjeljka
Eyring, Veronika
Atmospheric and Oceanic Physics
State-of-the-art Earth system models (ESMs) cannot explicitly resolve many small-scale atmospheric processes such as atmospheric gravity waves, and thus must represent, or parameterise, their effects on the resolved state. Machine learning (ML) has the potential to improve these parameterisations. In our study, we train neural networks (NNs) on ERA5 reanalysis data to predict momentum fluxes of orographic gravity waves as a function of the state variables at the resolution of a coarse ESM. Employing a full year of data, we extract inertia-gravity waves using the software MODES, which applies linear theory for wave filtering, and train ML models on data coarse-grained to the ESM's target resolution. We consider four different cases: the full spectrum of inertia-gravity waves resolved in ERA5, or just the part of the spectrum that is subgrid-scale in the target ESM, both over all land or just over mountainous terrain. Our NNs successfully predict momentum fluxes, with a global coefficient of determination ($R^2$) ranging from 0.72 to 0.56, depending on the case, when evaluated offline with data from another year. An analysis of our models using SHAP values, an explainable AI technique, suggests that the networks learned physically meaningful relationships. In addition, we give a comparison with the physics-based parameterisation scheme by Lott and Miller. This work forms the basis for the development of operational ML-based parameterisations to improve the representation of gravity waves and their effects in climate models.
title Interpretable Neural Networks to Predict Momentum Fluxes of Orographic Gravity Waves
topic Atmospheric and Oceanic Physics
url https://arxiv.org/abs/2605.05052