Corrigendum to: Evaluation of seasonal teleconnections to remote drivers of Australian rainfall in CMIP5 and CMIP6 models
Christine Chung , Ghyslaine Boschat , Andréa Taschetto , Sugata Narsey , Shayne McGregor , Agus Santoso and François DelageThis article corrects Journal of Southern Hemisphere Earth Systems Science 73(3), 219–261. doi:10.1071/ES23002
The authors regret to advise that seven models were formatted incorrectly in Table 1, which may cause confusion for some readers.
The table as published was as follows:
The five models with the highest spatial correlation between modelled and observed teleconnections, for each season.
| DJF | MAM | JJA | SON | ||
|---|---|---|---|---|---|
| ENSO (all years) | TaiESM1 | GFDL-CM4 | CESM2-FV2 | ACCESS-CM2 | |
| EC-Earth3-AerChem | MIROC6 | ACCESS-CM2 | E3SM1-1 | ||
| CAM5-CSM1-0 | GISS-E2-1-H | MIROC6 | E3SM1-1-ECA | ||
| IPSL-CM6A-LR-INCA | IPSL-CM6A-LR | NorCPM1 | CESM2-WACCM-FV2 | ||
| CESM2-WACCM-FV2 | NorESM2-MM | E3SM-1-0 | FGOALS-f3-L | ||
| La Niña years | CNRM-ESM2-1 | MCM-UA-1-0 | UKESM1-0-LL | IPSL-CM6A-LR-INCA | |
| E3SM-1-1 | GISS-E2-1-G-CC | TaiESM1 | MRI-ESM2-0 | ||
| CAMS-CMS1-0 | CAS-ESM2-0 | EC-Earth3 | E3SM-1-0 | ||
| TaiESM1 | IPSL-CM6A-LR | IPSL-CM6A-LR | TaiESM1 | ||
| CMCC-CM2-SR5 | GISS-E2-1-G | AWI-CM-1-1-MR | IPSL-CM6A-LR | ||
| El Niño years | CESM2-WACCM-FV2 | FGOALS-f3-L | BCC-ESM1 | BCC-ESM1 | |
| EC-Earth3-Veg-LR | EC-Earth3-AerChem | AWI-ESM-1-1-LR | EC-Earth3-CC | ||
| CESM2 | NESM3 | INM-CM5-0 | TaiESM1 | ||
| CESM2-WACCM | TaiESM1 | CESM2 | EC-Earth3-Veg | ||
| AWI-CM-1-1-MR | CESM2-WACCM-FV2 | ACCESS-CM2 | EC-Earth3-Veg-LR | ||
| IOD | E3SM-1-1-ECA | FGOALS-f3-L | |||
| FIO-ESM-2-0 | EC-Earth3-CC | ||||
| ACCESS-ESM1.5 | GFDL-ESM4 | ||||
| CESM2-WACCM | SAM0-UNICON | ||||
| GFDL-ESM4 | ACCESS-CM2 | ||||
| SAM | CESM2-FV2 | IPSL-CM6-LR-INCA | NESM3 | EC-Earth3-Veg-LR | |
| CIESM | MIROC-ES2L | AWI-CM-1-1-MR | E3SM-1-1-ECA | ||
| AWI-CM-1-1-MR | MPI-ESM1-2-HR | GISS-E2-1-H | EC-Earth3-AerChem | ||
| MPI-ESM1-2-LR | KACE-1-0-G | EC-Earth3-Veg | BCC-CSM2-MR | ||
| MIROC-ES2L | E3SM-1-1 | MPI-ESM2-1-2-HAM | CMCC-CM2-HR4 |
Models in bold were also selected as the downscaling choices in Grose et al. (2023), and models in italic are in the same family as the models in bold.
The formatting errors were: (1) CESM2-WACCM-FV2 should be italic not bold for ENSO (all years) and SON; (2) FGOALS-f3-L should be roman not bold for ENSO (all years) and SON; (3) GISS-E2-1-G should be roman not bold for La Niña years and MAM; (4) UKESM1-0-LL should be bold not roman for La Niña years and JJA; (5) MRI-ESM2-0 should be roman not bold for La Niña years and SON; (6) CMCC-CM2-SR5 should be italic not roman for La Niña years and DJF; and (7) CMCC-CM2-HR4 should be italic not roman for SAM and SON.
The table as it ought to be is as follows:
The five models with the highest spatial correlation between modelled and observed teleconnections, for each season.
| DJF | MAM | JJA | SON | ||
|---|---|---|---|---|---|
| ENSO (all years) | TaiESM1 | GFDL-CM4 | CESM2-FV2 | ACCESS-CM2 | |
| EC-Earth3-AerChem | MIROC6 | ACCESS-CM2 | E3SM1-1 | ||
| CAM5-CSM1-0 | GISS-E2-1-H | MIROC6 | E3SM1-1-ECA | ||
| IPSL-CM6A-LR-INCA | IPSL-CM6A-LR | NorCPM1 | CESM2-WACCM-FV2 | ||
| CESM2-WACCM-FV2 | NorESM2-MM | E3SM-1-0 | FGOALS-f3-L | ||
| La Niña years | CNRM-ESM2-1 | MCM-UA-1-0 | UKESM1-0-LL | IPSL-CM6A-LR-INCA | |
| E3SM-1-1 | GISS-E2-1-G-CC | TaiESM1 | MRI-ESM2-0 | ||
| CAMS-CMS1-0 | CAS-ESM2-0 | EC-Earth3 | E3SM-1-0 | ||
| TaiESM1 | IPSL-CM6A-LR | IPSL-CM6A-LR | TaiESM1 | ||
| CMCC-CM2-SR5 | GISS-E2-1-G | AWI-CM-1-1-MR | IPSL-CM6A-LR | ||
| El Niño years | CESM2-WACCM-FV2 | FGOALS-f3-L | BCC-ESM1 | BCC-ESM1 | |
| EC-Earth3-Veg-LR | EC-Earth3-AerChem | AWI-ESM-1-1-LR | EC-Earth3-CC | ||
| CESM2 | NESM3 | INM-CM5-0 | TaiESM1 | ||
| CESM2-WACCM | TaiESM1 | CESM2 | EC-Earth3-Veg | ||
| AWI-CM-1-1-MR | CESM2-WACCM-FV2 | ACCESS-CM2 | EC-Earth3-Veg-LR | ||
| IOD | E3SM-1-1-ECA | FGOALS-f3-L | |||
| FIO-ESM-2-0 | EC-Earth3-CC | ||||
| ACCESS-ESM1.5 | GFDL-ESM4 | ||||
| CESM2-WACCM | SAM0-UNICON | ||||
| GFDL-ESM4 | ACCESS-CM2 | ||||
| SAM | CESM2-FV2 | IPSL-CM6-LR-INCA | NESM3 | EC-Earth3-Veg-LR | |
| CIESM | MIROC-ES2L | AWI-CM-1-1-MR | E3SM-1-1-ECA | ||
| AWI-CM-1-1-MR | MPI-ESM1-2-HR | GISS-E2-1-H | EC-Earth3-AerChem | ||
| MPI-ESM1-2-LR | KACE-1-0-G | EC-Earth3-Veg | BCC-CSM2-MR | ||
| MIROC-ES2L | E3SM-1-1 | MPI-ESM2-1-2-HAM | CMCC-CM2-HR4 |
Models in bold were also selected as the downscaling choices in Grose et al. (2023), and models in italic are in the same family as the models in bold.
