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Peer-reviewedCC BYJournal of Advances in Modeling Earth Systems

The Ensemble Kalman Inversion Race

  1. 1Cecil H. and Ida M. Green Institute of Geophysics and Planetary Physics Scripps Institution of Oceanography University of California San Diego San Diego CA USA
  2. 2California Institute of Technology Pasadena CA USA

Abstract

Ensemble Kalman methods were initially developed to solve nonlinear data assimilation problems in oceanography but are now popular in applications far beyond their original use cases. Of particular interest is climate model calibration. As hybrid physics and machine‐learning models advance, the number of parameters and complexity of parameterizations in climate models will continue to grow. To fully realize these advances, we must move from laborious hand‐tuning to calibration‐driven model development in rapid iteration cycles. Thus, robust calibration of these parameters plays an increasingly important role. We focus on learning climate model parameters by minimizing the misfit between modeled and observed climate statistics in an idealized setting. Ensemble Kalman methods are a natural choice for this problem because they are derivative‐free, scalable to high dimensions, and robust to noise caused by statistical observations. Given the many variants of ensemble methods proposed, an important question is: Which ensemble Kalman method should be used for climate model calibration ? To answer this question, we perform systematic numerical experiments to explore the relative computational efficiencies of several ensemble Kalman methods. The numerical experiments involve statistical observations of Lorenz‐type models of increasing complexity, frequently used to represent simplified atmospheric systems, with some featuring neural network parameterizations. For each test problem, several ensemble Kalman methods and a derivative‐based method “race” to reach a specified accuracy, and we measure the computational cost required to achieve the desired accuracy. We investigate how prior information and the parameter or data dimensions define the computational costs of the various methods.

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BibTeX
@article{gjini2026ensemble,
  title = {{The Ensemble Kalman Inversion Race}},
  author = {Rebecca Gjini and Matthias Morzfeld and Oliver R. A. Dunbar and Tapio Schneider},
  journal = {Journal of Advances in Modeling Earth Systems},
  year = {2026},
  month = sep,
  doi = {10.1029/2025ms005629},
  url = {https://doi.org/10.1029/2025ms005629},
  note = {CC BY},
}
RIS
TY  - JOUR
TI  - The Ensemble Kalman Inversion Race
AU  - Rebecca Gjini
AU  - Matthias Morzfeld
AU  - Oliver R. A. Dunbar
AU  - Tapio Schneider
PY  - 2026
DA  - 2026/09/01
JO  - Journal of Advances in Modeling Earth Systems
DO  - 10.1029/2025ms005629
UR  - https://doi.org/10.1029/2025ms005629
AB  - Ensemble Kalman methods were initially developed to solve nonlinear data assimilation problems in oceanography but are now popular in applications far beyond their original use cases. Of particular interest is climate model calibration. As hybrid physics and machine‐learning models advance, the number of parameters and complexity of parameterizations in climate models will continue to grow. To fully realize these advances, we must move from laborious hand‐tuning to calibration‐driven model development in rapid iteration cycles. Thus, robust calibration of these parameters plays an increasingly important role. We focus on learning climate model parameters by minimizing the misfit between modeled and observed climate statistics in an idealized setting. Ensemble Kalman methods are a natural choice for this problem because they are derivative‐free, scalable to high dimensions, and robust to noise caused by statistical observations. Given the many variants of ensemble methods proposed, an important question is: Which ensemble Kalman method should be used for climate model calibration ? To answer this question, we perform systematic numerical experiments to explore the relative computational efficiencies of several ensemble Kalman methods. The numerical experiments involve statistical observations of Lorenz‐type models of increasing complexity, frequently used to represent simplified atmospheric systems, with some featuring neural network parameterizations. For each test problem, several ensemble Kalman methods and a derivative‐based method “race” to reach a specified accuracy, and we measure the computational cost required to achieve the desired accuracy. We investigate how prior information and the parameter or data dimensions define the computational costs of the various methods.
SN  - 1942-2466
ER  -