the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Using Probabilistic Machine Learning to Better Model Temporal Patterns in Parameterizations: a case study with the Lorenz 96 model
Abstract. The modelling of small-scale processes is a major source of error in climate models, hindering the accuracy of low-cost models which must approximate such processes through parameterization. Red noise is essential to many operational parameterization schemes, helping model temporal correlations. We show how to build on the successes of red noise by combining the known benefits of stochasticity with machine learning. This is done using a physically-informed recurrent neural network within a probabilistic framework. Our model is competitive and often superior to both a bespoke baseline and an existing probabilistic machine learning approach (GAN) when applied to the Lorenz 96 atmospheric simulation. This is due to its superior ability to model temporal patterns compared to standard first-order autoregressive schemes. It also generalises to unseen scenarios. We evaluate across a number of metrics from the literature, and also discuss the benefits of using the probabilistic metric of hold-out likelihood.
-
Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
-
Preprint
(1338 KB)
-
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(1338 KB) - Metadata XML
- BibTeX
- EndNote
- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
-
RC1: 'Comment on egusphere-2022-912', Anonymous Referee #1, 05 Nov 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-912/egusphere-2022-912-RC1-supplement.pdf
-
RC2: 'Comment on egusphere-2022-912', Pavel Perezhogin, 04 Mar 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-912/egusphere-2022-912-RC2-supplement.pdf
-
AC1: 'Comment on egusphere-2022-912', Raghul Parthipan, 25 Apr 2023
We would like to thank both our reviewers for taking the time to provide such great in-depth comments and suggestions. We have made the appropriate changes and believe the manuscript is notably improved as a result. We have attached a supplement which includes a summary of the changes we have made, and notes to address specific comments from each reviewer.
Interactive discussion
Status: closed
-
RC1: 'Comment on egusphere-2022-912', Anonymous Referee #1, 05 Nov 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-912/egusphere-2022-912-RC1-supplement.pdf
-
RC2: 'Comment on egusphere-2022-912', Pavel Perezhogin, 04 Mar 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-912/egusphere-2022-912-RC2-supplement.pdf
-
AC1: 'Comment on egusphere-2022-912', Raghul Parthipan, 25 Apr 2023
We would like to thank both our reviewers for taking the time to provide such great in-depth comments and suggestions. We have made the appropriate changes and believe the manuscript is notably improved as a result. We have attached a supplement which includes a summary of the changes we have made, and notes to address specific comments from each reviewer.
Peer review completion
Journal article(s) based on this preprint
Model code and software
Model code Raghul Parthipan https://zenodo.org/record/7118668
Viewed
HTML | XML | Total | BibTeX | EndNote | |
---|---|---|---|---|---|
625 | 161 | 15 | 801 | 4 | 5 |
- HTML: 625
- PDF: 161
- XML: 15
- Total: 801
- BibTeX: 4
- EndNote: 5
Viewed (geographical distribution)
Country | # | Views | % |
---|
Total: | 0 |
HTML: | 0 |
PDF: | 0 |
XML: | 0 |
- 1
Hannah M. Christensen
J. Scott Hosking
Damon J. Wischik
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(1338 KB) - Metadata XML