Abstract

The impact of stochastic physics on El Niño Southern Oscillation (ENSO) is investigated in the EC-Earth coupled climate model. By comparing an ensemble of three members of control historical simulations with three ensemble members that include stochastics physics in the atmosphere, we find that in EC-Earth the implementation of stochastic physics improves the excessively weak representation of ENSO. Specifically, the amplitude of both El Niño and, to a lesser extent, La Niña increases. Stochastic physics also ameliorates the temporal variability of ENSO at interannual time scales, demonstrated by the emergence of peaks in the power spectrum with periods of 5–7 years and 3–4 years. Based on the analogy with the behaviour of an idealized delayed oscillator model (DO) with stochastic noise, we find that when the atmosphere–ocean coupling is small (large) the amplitude of ENSO increases (decreases) following an amplification of the noise amplitude. The underestimated ENSO variability in the EC-Earth control runs and the associated amplification due to stochastic physics could be therefore consistent with an excessively weak atmosphere–ocean coupling. The activation of stochastic physics in the atmosphere increases westerly wind burst (WWB) occurrences (i.e. amplification of noise amplitude) that could trigger more and stronger El Niño events (i.e. increase of ENSO oscillation) in the coupled EC-Earth model. Further analysis of the mean state bias of EC-Earth suggests that a cold sea surface temperature (SST) and dry precipitation bias in the central tropical Pacific together with a warm SST and wet precipitation bias in the western tropical Pacific are responsible for the coupled feedback bias (weak coupling) in the tropical Pacific that is related to the weak ENSO simulation. The same analysis of the ENSO behaviour is carried out in a future scenario experiment (RCP8.5 forcing), highlighting that in a coupled model with an extreme warm SST, characterized by a strong coupling, the effect of stochastic physics on the ENSO representation is opposite. This corroborates the hypothesis that the mean state bias of the tropical Pacific region is the main reason for the ENSO representation deficiency in EC-Earth.

Highlights

  • The El Niño Southern Oscillation (ENSO) is the most prominent phenomenon in the tropical Pacific Ocean at interannual time scales (Rasmusson and Carpenter 1982)

  • In order to evaluate the impact of stochastic physics on ENSO, first we calculate the composite of El Niño and La Niña events for the period of 1870–2009

  • In CCSM was attributed to these observed impacts on westerly wind burst (WWB), and it was suggested that a systematic reduction on the atmosphere–ocean coupling strength observed in the La Niña phase was the primary cause of the reduced ENSO amplitude in CCSM (Christensen et al 2017)

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Summary

Introduction

The El Niño Southern Oscillation (ENSO) is the most prominent phenomenon in the tropical Pacific Ocean at interannual time scales (Rasmusson and Carpenter 1982). In this theory the equatorial heat content is discharged (recharged) during a warm (cold) ENSO phase due to mass exchange between equatorial and off-equatorial regions associated with central Pacific wind anomalies and eastern Pacific Sea Surface Temperature (SST) anomalies (see Jin 1997a, b) Another key aspect of ENSO theory concerns the role of stochastic forcing, which has been widely discussed in several studies. One recent important breakthrough for numerical weather prediction models was the development of stochastic parameterization schemes at the European Centre for MediumRange Weather Forecasts (ECMWF) (Palmer et al 2009; Buizza et al 1999) These schemes represent the variability of unresolved atmospheric processes.

Data and methods
The response of ENSO to stochastic physics
Delayed oscillator
The impact of stochastic physics on WWBs
Assessing atmosphere–ocean coupling strength using a statistical model
The mean state of the tropical Pacific Ocean
Discussions and conclusions
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