Interpretable multiscale Machine Learning-Based Parameterizations of Convection for ICON
Helge Heuer, Mierk Schwabe, Pierre Gentine, Marco A. Giorgetta,, Veronika Eyring

TL;DR
This study develops and benchmarks machine learning-based parameterizations for convection in the ICON Earth System Model, demonstrating improved simulation of precipitation extremes and stability over traditional schemes.
Contribution
It introduces a multiscale, interpretable ML approach using U-Net architectures for convection parameterization in a realistic Earth system model setting.
Findings
A U-Net model outperforms other ML algorithms offline.
The ablated U-Net improves precipitation extremes simulation.
Online, the ablated U-Net enhances model stability.
Abstract
Machine learning (ML)-based parameterizations have been developed for Earth System Models (ESMs) with the goal to better represent subgrid-scale processes or to accelerate computations. ML-based parameterizations within hybrid ESMs have successfully learned subgrid-scale processes from short high-resolution simulations. However, most studies used a particular ML method to parameterize the subgrid tendencies or fluxes originating from the compound effect of various small-scale processes (e.g., radiation, convection, gravity waves) in mostly idealized settings or from superparameterizations. Here, we use a filtering technique to explicitly separate convection from these processes in simulations with the Icosahedral Non-hydrostatic modelling framework (ICON) in a realistic setting and benchmark various ML algorithms against each other offline. We discover that an unablated U-Net, while…
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Taxonomy
TopicsClimate variability and models · Meteorological Phenomena and Simulations · Oceanographic and Atmospheric Processes
