4.7 Article

Key Role of Diabatic Processes in Regulating Warm Water Volume Variability over ENSO Events

期刊

JOURNAL OF CLIMATE
卷 33, 期 22, 页码 9945-9964

出版社

AMER METEOROLOGICAL SOC
DOI: 10.1175/JCLI-D-20-0198.1

关键词

Dynamics; ENSO; Ocean circulation; Diabatic heating; Climate models; Interannual variability

资金

  1. Australian Research Council
  2. ARC Centre of Excellence for Climate Extremes [FL150100090]
  3. Centre for Southern Hemisphere Oceans Research (CSHOR)

向作者/读者索取更多资源

The equatorial Pacific warm water volume (WWV), defined as the volume of water warmer than 20 degrees C near the equator, is a keyy predictor for El Nino-Southern Oscillation (ENSO), and yet much about the individual processes that influence it remains unknown. In this study, we conduct idealized ENSO simulations forced with symmetric El Nino- and La Nina-associated atmospheric anomalies as well as a historical 1979-2016 hindcast simulation. We use the water mass transformation framework to examine the individual contributions of diabatic and adiabatic processes to changes in WWV. We find that in both sets of simulations, El Nino's discharge and La Nina's recharge periods are initiated by diabatic fluxes of volume across the 20 degrees C isotherm associated with changes in surface forcing and vertical mixing. Changes in adiabatic horizontal volume transport above 20 degrees C between the equator and subtropical latitudes dominate at a later stage. While surface forcing and vertical mixing deplete WWV during El Nino, surface forcing during La Nina drives a large increase partially compensated for by a decrease driven by vertical mixing. On average, the ratio of diabatic to adiabatic contributions to changes in WWV during El Nino is about 40% to 60%; during La Nina this ratio changes to 75% to 25%. The increased importance of the diabatic processes during La Nina, especially the surface heat fluxes, is linked to the shoaling of the 20 degrees C isotherm in the eastern equatorial Pacific and is a major source of asymmetry between the two ENSO phases, even in the idealized simulations where the wind forcing and adiabatic fluxes are symmetric.

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