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Schematic diagrams for (a)-(d) CT ENSO and (e)-(h) WP ENSO recharge oscillator mechanisms in the (a),(e) warm, (b),(f) warm-to-cold, (c),(h) cold, and (d),(g) cold-to-warm phases. The red (blue) shadings on the top planes representing the sea surface denote positive (negative) SST anomalies, and those on the inclined planes representing the climatic thermocline denote positive (negative) subsurface temperature anomalies. The dark gray arrows denote mean upwelling,; the black arrows represent the zonal and meridional upper-ocean geostrophic current anomalies, and the solid yellow arrows stand for wind stress anomalies: W, C, H, and L denote warm, cold, high, and low, respectively. 

Schematic diagrams for (a)-(d) CT ENSO and (e)-(h) WP ENSO recharge oscillator mechanisms in the (a),(e) warm, (b),(f) warm-to-cold, (c),(h) cold, and (d),(g) cold-to-warm phases. The red (blue) shadings on the top planes representing the sea surface denote positive (negative) SST anomalies, and those on the inclined planes representing the climatic thermocline denote positive (negative) subsurface temperature anomalies. The dark gray arrows denote mean upwelling,; the black arrows represent the zonal and meridional upper-ocean geostrophic current anomalies, and the solid yellow arrows stand for wind stress anomalies: W, C, H, and L denote warm, cold, high, and low, respectively. 

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... The SSHA and sea current anomaly changes in the eastern Pacific are relatively weaker and slower than those in the central Pacific ( Figures 8B,G), and the poleward Sverdrup transports show less inter-hemispheric asymmetry ( Figure 9B). These oceanic responses to the SWS and the associated negative oceanic feedback are consistent with those revealed by Ren and Jin (2013) that the reversal of the equatorial sea current anomalies provides the initial negative feedback for El Niño phase transition. ...
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... The mentioned feedbacks were shown to contribute differently to the generation of two El Niño types. The thermocline feedback plays a key role in the evolution of El Niño events with the maximum SSTA variability in the eastern Pacific, while the zonal advective feedback is responsible for SSTA growth in the central Pacific [9,[13][14][15]. Zonal advective feedback also plays an important role in the development of strong El Niño events [16], being an important contributor to the SSTA growth both in the central and eastern Pacific [14,17]. ...
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The heat budget of the equatorial Pacific mixed layer during El Niño formation was studied based on reanalysis (GLORYS2V4) and model data for the modern climate. The focus of the study is on the so-called El Niño diversity, i.e., the existence of different types of events that are characterized by different locations and intensities, as well as significantly different teleconnection all around the world. The analysis of the processes that participate in the formation of different El Niño types may serve for a better understanding of the El Niño dynamic and contribute to improving its forecast. Two classifications, based on the location and intensity of the events, were considered: strong/moderate and Eastern Pacific (EP)/Central Pacific (CP). The analysis did not reveal a significant difference in the heat budget of the mixed layer between strong and EP El Niño events, as well as between moderate and CP events. The major difference in the generation mechanism of strong (EP) and moderate (CP) El Niño events consists of the magnitude of heating produced by ocean heat budget components with higher heating rates for strong (EP) events. The evolution of sea surface temperature anomalies (SSTA) is governed primarily by oceanic advection. The vertical advection (due to the thermocline feedback) is the main contributor to SSTA growth in the eastern Pacific regardless of El Niño’s type. In the Central Pacific, horizontal advection is more important than vertical one, with a stronger impact of meridional processes for both strong and moderate regimes. Furthermore, the evaluation of the CMIP5 model’s skill in the simulation of the processes responsible for the formation of different El Niño types was carried out. The analysis of the heat budget of the mixed layer in the CMIP5 ensemble demonstrated that the most successful models are CCSM4, CESM1-BGC, CMCC-CMS, CNRM-CM5, GFDL-ESM2M, and IPSL-CM5B-LR. They are capable of reproducing the most important contribution of the advection terms in the SSTA tendency, keeping the major role of the thermocline feedback (and vertical advection) in the eastern Pacific, and do not overestimate the contribution of zonal advective feedback. These models are recommended to be used for the analysis of El Niño mechanism modification in the future climate.
... To diagnose the specific contributions of different dynamical processes to the ocean temperature anomaly during El Niño evolution, a mixed-layer heat budget analysis (An et al., 1999;Kug et al., 2009;Li et al., 2002;Zhang et al., 2007) was conducted. Following the definition by Ren and Jin (2013), the equation for the mixed-layer temperature anomaly tendency (MLTAT), consisting of six feedback terms and a residual term (R), can be expressed as ...
... According to previous studies, ZA is an essential oceanic dynamical process that controls the ENSO growth rate (Jin & Neelin, 1993;Ren & Jin, 2013;Zhang et al., 2007). Hence, this feedback attributed to the biased structure of ZCA might hinder the models' ability to simulate a realistic El Niño evolution. ...
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