Abstract

El Niño Southern Oscillation (ENSO) is the leading mode of tropical Pacific variability at interannual timescales. Through atmospheric teleconnections, ENSO exerts large influences worldwide, so that improved understanding of this phenomenon can be of critical societal relevance. Extreme ENSO events, in particular, have been associated with devastating weather events in many parts of the world, so that the ability to assess their frequency and probability of occurrence is extremely important. In this study, we describe the ENSO phenomenon in terms of the Recharge Oscillator Model perturbed by multiplicative deterministic chaotic forcing, and use methodologies from the field of Statistical Mechanics to determine the average time between El Niño events of given strengths. This is achieved by describing the system in terms of its probability density function, which is governed by a Fokker Planck equation, and then using the Mean First Passage Time technique for the determination of the mean time between extreme events. The ability to obtain analytical solutions to the problem allows a clear identification of the most relevant model parameters for controlling the frequency of extreme events. The key parameter is the strength of the multiplicative component of the stochastic perturbation, but the decorrelation timescale of the stochastic forcing is also very influential. Results obtained with this approach suggest an average waiting time between extreme events of only some tens of years.

Highlights

  • In spite of this complexity, simple dynamical paradigms have been able to describe the basic features of ENSO by capturing essential aspects of the system.In particular, the “recharge oscillator” model (ROM)[4,5] focuses on the recharge/discharge of the equatorial Pacific upper-ocean warm water volume

  • We extend the results of B_16 to examine the average time between events of a given amplitude, by using the mean First Passage Time (FPT) technique, a method stemming from the field of statistical mechanics

  • As in B_16, using a projection/perturbation approach, we obtain a generalized FokkerPlanck Equation (FPE) for the Probability Density Function (PDF) of the ROM, from which, adapting the standard FPT procedures to this nonstandard case, we get analytical expressions for the average time between strong events and for its associated standard deviation

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Summary

INTRODUCTION

In spite of this complexity, simple dynamical paradigms (or Low Order Models—LOM) have been able to describe the basic features of ENSO by capturing essential aspects of the system (see Ref. 3). An alternative approach for the inclusion of fast state-dependent perturbations to the recharge oscillator model is the projective method of Bianucci,[20,21,22,23] adapted to the ROM case[24] (B_16 hereafter), where the system is described in terms of its Probability Density Function (PDF) governed by a FokkerPlanck Equation (FPE), for which analytical solutions can be obtained. We extend the results of B_16 to examine the average time between events of a given amplitude, by using the mean First Passage Time (FPT) technique, a method stemming from the field of statistical mechanics This quantity, for which an analytical expression can be determined, is of particular interest in the case of extreme events. A deeper discussion about the affective and respective roles of the dimension and of the nonlinearities of a LOM to model the complexity of ENSO goes beyond the task of the present work

THE DYNAMICAL MODEL AND THE FPE
THE STATIONARY PDF
THE MEAN FPT FOR ENSO EVENTS
CONCLUSION
The formal approach
The general FPE for the ROM
The dynamics of the first two moments
The ansatz at work for the calculation of the FPT
Findings
Analytic expression for the mean FPT
Full Text
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