Journal cover Journal topic
Climate of the Past An interactive open-access journal of the European Geosciences Union
https://doi.org/10.5194/cp-2016-128
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
Research article
19 Jan 2017
Review status
This discussion paper is a preprint. It has been under review for the journal Climate of the Past (CP). The revised manuscript was not accepted.
Evolution and forcing mechanisms of ENSO over the last 300,000 years in CCSM3
Zhengyao Lu1, Zhengyu Liu1,2, Guangshan Chen2, and Jian Guan1 1Lab. Climate, Ocean and Atmosphere Studies, School of Physics, Peking Univ., Beijing, 100871, P. R. China
2Dept. Atmospheric and Oceanic Sciences & Nelson Center for Climatic Research, Univ. of Wisconsin-Madison, Madison, WI53706, USA
Abstract. The responses of El Niño-Southern Oscillation (ENSO) and the equatorial Pacific annual cycle to external forcing changes are studied in three 3,000-year-long NCAR-CCSM3 model simulations. The simulations represent the period from 300 thousand years before present (ka BP) to present day. The first idealized simulation is forced only with accelerated orbital variations, and the rest are conducted more realistically by further adding on the time-varying boundary conditions of greenhouse gases (GHGs) and continental ice sheets.

It is found that orbital forcing dominates slow ENSO evolution, while the effects of GHGs and ice-sheet forcing tend to compensate each other. On the orbital time scales, ENSO variability and annual cycle amplitude change in-phase and both have pronounced precessional cycles (~ 21,000 years) modulated by variations of eccentricity. Orbital forced ENSO intensity is dominated linearly by the change of the coupled ocean-atmosphere instability, notably the Ekman upwelling feedback and the thermocline feedback; and is also possibly affected during ENSO intrinsic developing season by the remote (or extratropical) influences of the short-scale stochastic weather noises. The acceleration technique is found to dampen the precessional signal in ENSO intensity.

In glacial-interglacial cycles, additionally, the weakening/strengthening of ENSO owning to a more concentrated/depleted GHGs level leaves little net signal as compensated by the effect coherent change of decaying/expanding ice sheets. They influence the ENSO variability through changes in annual cycle amplitude via a common nonlinear frequency entrainment mechanism while the GHGs effect might has an additional linear part.


Citation: Lu, Z., Liu, Z., Chen, G., and Guan, J.: Evolution and forcing mechanisms of ENSO over the last 300,000 years in CCSM3, Clim. Past Discuss., https://doi.org/10.5194/cp-2016-128, 2017.
Zhengyao Lu et al.
Interactive discussionStatus: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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RC1: 'Review of ``Evolution and forcing mechanisms of ENSO over the last 300,000 years in CCSM3'' by Lu et al', Anonymous Referee #1, 03 Mar 2017 Printer-friendly Version 
 
RC2: 'Review of manuscript', Anonymous Referee #2, 18 Apr 2017 Printer-friendly Version 
 
AC1: 'Response to Reviewers' Comments', Zhengyao Lu, 29 May 2017 Printer-friendly Version Supplement 
Zhengyao Lu et al.
Zhengyao Lu et al.

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Short summary
We use complex climate model simulations to study how the intensity of El Niño-Southern Oscillation (ENSO) changed for the last 300 thousand years. We consider external climatic forcings like orbital variations, greenhouse gases and ice-sheets. We find that orbital forcing dominates slow ENSO evolution by modulating the change of the coupled ocean-atmosphere instability, while the effects of GHGs and ice-sheet forcing tend to compensate each other.
We use complex climate model simulations to study how the intensity of El Niño-Southern...
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