The Pacific–Indian Ocean associated mode in CMIP5 models

The Pacific–Indian Ocean associated mode (PIOAM), defined as the first dominant mode (empirical orthogonal function, EOF1) of sea surface temperature anomalies (SSTAs) in the Pacific–Indian Ocean between 20 ∘ S and 20 ∘ N, is the product of the tropical air–sea interaction at the cross-basin scale a...

Full description

Bibliographic Details
Published in:Ocean Science
Main Authors: Yang, Minghao, Li, Xin, Shi, Weilai, Zhang, Chao, Zhang, Jianqi
Format: Text
Language:English
Published: 2020
Subjects:
Online Access:https://doi.org/10.5194/os-16-469-2020
https://os.copernicus.org/articles/16/469/2020/
id ftcopernicus:oai:publications.copernicus.org:os75578
record_format openpolar
spelling ftcopernicus:oai:publications.copernicus.org:os75578 2023-05-15T18:18:46+02:00 The Pacific–Indian Ocean associated mode in CMIP5 models Yang, Minghao Li, Xin Shi, Weilai Zhang, Chao Zhang, Jianqi 2020-04-23 application/pdf https://doi.org/10.5194/os-16-469-2020 https://os.copernicus.org/articles/16/469/2020/ eng eng doi:10.5194/os-16-469-2020 https://os.copernicus.org/articles/16/469/2020/ eISSN: 1812-0792 Text 2020 ftcopernicus https://doi.org/10.5194/os-16-469-2020 2020-07-20T16:22:14Z The Pacific–Indian Ocean associated mode (PIOAM), defined as the first dominant mode (empirical orthogonal function, EOF1) of sea surface temperature anomalies (SSTAs) in the Pacific–Indian Ocean between 20 ∘ S and 20 ∘ N, is the product of the tropical air–sea interaction at the cross-basin scale and the main mode of ocean variation in the tropics. Evaluating the capability of current climate models to simulate the PIOAM and finding the possible factors that affect the simulation results are beneficial in the pursuit of more accurate future climate change prediction. Based on the 55-year Hadley Centre Global Sea Ice and Sea Surface Temperature (HadISST) dataset and the output data from 21 Coupled Model Intercomparison Project (CMIP) phase 5 (CMIP5) models, the PIOAM in these CMIP5 models is assessed. Instead of using the time coefficient (PC1) of the PIOAM as its index, we chose to utilize the alternative PIOAM index (PIOAMI), defined with SSTA differences in the boxes, to describe the PIOAM. It is found that the explained variance of the PIOAM in almost all 21 CMIP5 models is underestimated. Although all models reproduce the spatial pattern of the positive sea surface temperature anomaly in the eastern equatorial Pacific well, only one-third of these models successfully simulate the El Niño–Southern Oscillation (ENSO) mode with the east–west inverse phase in the Pacific Ocean. In general, CCSM4, GFDL-ESM2M and CMCC-CMS have a stronger capability to capture the PIOAM than the other models. The strengths of the PIOAM in the positive phase in less than one-fifth of the models are slightly greater, and very close to the HadISST dataset, especially CCSM4. The interannual variation of the PIOAM can be measured by CCSM4, GISS-E2-R and FGOALS-s2. Text Sea ice Copernicus Publications: E-Journals Indian Pacific Ocean Science 16 2 469 482
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The Pacific–Indian Ocean associated mode (PIOAM), defined as the first dominant mode (empirical orthogonal function, EOF1) of sea surface temperature anomalies (SSTAs) in the Pacific–Indian Ocean between 20 ∘ S and 20 ∘ N, is the product of the tropical air–sea interaction at the cross-basin scale and the main mode of ocean variation in the tropics. Evaluating the capability of current climate models to simulate the PIOAM and finding the possible factors that affect the simulation results are beneficial in the pursuit of more accurate future climate change prediction. Based on the 55-year Hadley Centre Global Sea Ice and Sea Surface Temperature (HadISST) dataset and the output data from 21 Coupled Model Intercomparison Project (CMIP) phase 5 (CMIP5) models, the PIOAM in these CMIP5 models is assessed. Instead of using the time coefficient (PC1) of the PIOAM as its index, we chose to utilize the alternative PIOAM index (PIOAMI), defined with SSTA differences in the boxes, to describe the PIOAM. It is found that the explained variance of the PIOAM in almost all 21 CMIP5 models is underestimated. Although all models reproduce the spatial pattern of the positive sea surface temperature anomaly in the eastern equatorial Pacific well, only one-third of these models successfully simulate the El Niño–Southern Oscillation (ENSO) mode with the east–west inverse phase in the Pacific Ocean. In general, CCSM4, GFDL-ESM2M and CMCC-CMS have a stronger capability to capture the PIOAM than the other models. The strengths of the PIOAM in the positive phase in less than one-fifth of the models are slightly greater, and very close to the HadISST dataset, especially CCSM4. The interannual variation of the PIOAM can be measured by CCSM4, GISS-E2-R and FGOALS-s2.
format Text
author Yang, Minghao
Li, Xin
Shi, Weilai
Zhang, Chao
Zhang, Jianqi
spellingShingle Yang, Minghao
Li, Xin
Shi, Weilai
Zhang, Chao
Zhang, Jianqi
The Pacific–Indian Ocean associated mode in CMIP5 models
author_facet Yang, Minghao
Li, Xin
Shi, Weilai
Zhang, Chao
Zhang, Jianqi
author_sort Yang, Minghao
title The Pacific–Indian Ocean associated mode in CMIP5 models
title_short The Pacific–Indian Ocean associated mode in CMIP5 models
title_full The Pacific–Indian Ocean associated mode in CMIP5 models
title_fullStr The Pacific–Indian Ocean associated mode in CMIP5 models
title_full_unstemmed The Pacific–Indian Ocean associated mode in CMIP5 models
title_sort pacific–indian ocean associated mode in cmip5 models
publishDate 2020
url https://doi.org/10.5194/os-16-469-2020
https://os.copernicus.org/articles/16/469/2020/
geographic Indian
Pacific
geographic_facet Indian
Pacific
genre Sea ice
genre_facet Sea ice
op_source eISSN: 1812-0792
op_relation doi:10.5194/os-16-469-2020
https://os.copernicus.org/articles/16/469/2020/
op_doi https://doi.org/10.5194/os-16-469-2020
container_title Ocean Science
container_volume 16
container_issue 2
container_start_page 469
op_container_end_page 482
_version_ 1766195460863688704