Skip to content

JGCRI/SnyderEtAl2023_uncertainty_informed_curation_metarepo

Folders and files

NameName
Last commit message
Last commit date

Latest commit

 

History

14 Commits
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 

Repository files navigation

DOI

SnyderEtAl2023_uncertainty_informed_curation_metarepo

Uncertainty-informed selection of CMIP6 Earth System Model subsets for use in multisectoral and impact models

Abigail Snyder1*, Noah Prime1, Claudia Tebaldi1, and Kalyn Dorheim1

1 Joint Global Change Research Institute, Pacific Northwest National Laboratory and University of Maryland, College Park, MD

* corresponding author: [email protected]

Abstract

Earth System Models (ESMs) are heavily used to provide inputs to specific impact and multisectoral dynamic models. Therefore, representing the full range of model uncertainty, scenario uncertainty, and interannual variability that ensembles of ESMs capture , is critical to the exploration of the future co-evolution of the integrated human-Earth system. The pre-eminent source of these ensembles has been the Coupled Model Intercomparison Project (CMIP) however, the increased participation by modeling centers in every new phase of CMIP relative to previous eras results in increasingly large archives of ESM data that can be intractable for impact modelers to effectively utilize, due to computational constraints and the challenges of analyzing large datasets. In this work, we describe a method to select a subset of the latest phase, CMIP6, models for use as inputs to a sectoral impact or multisectoral model, while still representing the range of model uncertainty, scenario uncertainty, and interannual variability of the full CMIP6 ESM results. This method is intended to help human-relevant impact and multisectoral modelers select climate information from the CMIP archive efficiently. This is particularly critical for large ensemble experiments of multisectoral dynamic models that may be varying additional features beyond climate inputs in a factorial design, thus putting constraints on the number of climate simulations that can be used. We focus on temperature and precipitation outputs of ESMs, as these are two of the most used variables among impact models and many other key input variables for impacts are at least correlated with one or both of temperature and precipitation (e.g. relative humidity). Besides preserving the multi-model ensemble variance characteristics, we prioritize selecting ESMs in the subset that preserve the very likely distribution of equilibrium climate sensitivity values as assessed by the latest IPCC report. This approach could be applied to other output variables of ESMs and, when combined with emulators, offers a flexible framework for designing more efficient experiments on human-relevant climate impacts. It can also provide greater insight into the properties of existing ESMs and the method may be informative for future experiment planning across ESMs.

This repository collects code for the calculations performed in this paper.

Journal reference

Submitted to Earth System Dynamics

Workflow

Run the following scripts to re-create the manuscript experiments:

Script Name Description
aoi_extractions.py Script that processes NetCDF gridded time series data of multiple variables (T, P) to time series of annual average values in each of the IPCC WGI regions.
metric_calc.ipynb Script that processes annual T, P time series data in each IPCC region to the six summary metrics of interest described in the paper.
climate_sensitivity_sampling.ipynb Script that takes a subset of 5 ESMs from a provided list that preserve the IPCC very likely distribution of ECS values.
subset_selection.Rmd Script that 1. performs PCA decomposition of the full set of ScenarioMIP Tier 1 participating ESMs. 2. Identifies the optimal subset of ECS-distribution-preserving ESMs to span the reduced dimension space found by the PCA.
subset_selection.html An executed copy of subset_selection.Rmd
separating_uncertainty.ipynb Script that calculates the Hawkins and Sutton uncertainty partitions for the first available ensemble member for T and P for both the full set CMIP6 ESMs and a specified subset
HS-uncertainty-evaluation.Rmd Script that compares the Hawkins and Sutton uncertainty partitions for the first available ensemble member for T and P for both the full set CMIP6 ESMs and selected subset, for validation purposes.
HS-uncertainty-evaluation.html An executed copy of HS-uncertainty-evaluation.Rmd

Data generated for this publication are archived ().

About

No description, website, or topics provided.

Resources

Stars

Watchers

Forks

Releases

No releases published

Packages

No packages published