The El Niño-Southern Oscillation (ENSO) is a climate phenomenon that recurs about every 2-7 yr between its warm (El Niño) and cold (La Niña) phases across the equatorial Pacific, strongly affecting global climate and environment (e.g., McPhaden et al., 2006;Timmermann et al., 2018). It is commonly viewed as a low-frequency coupled ocean-atmosphere mode energized by stochastic wind forcing, with its growth and phase transition originating from the combination of the positive ocean-atmosphere instability and the delayed negative oceanic feedbacks (Bjerknes, 1969;Cane & Zebiak, 1985;Neelin et al., 1998;Wyrtki, 1985). Jin's (1997aJin's ( , 1997b recharge oscillator (RO), the simplest possible paradigm for ENSO, incorporates these feedback processes involving sea surface temperature (SST), zonal wind stress, and thermocline depth (20°C isotherm depth, D20) and depicts ENSO phase transition as a result of the slow recharge/discharge of equatorial upper-ocean heat content (also known as warm water volume above D20; WWV). This paradigm has been substantiated in the observations, showing that basinwide WWV anomalies lead ENSO SST anomalies by about one to three seasons (Meinen & McPhaden, 2000), making WWV a good ENSO predictor (Clarke & Van Gorder, 2003;McPhaden, 2003). The anomalous western equatorial Pacific WWV (WWV w ), which was highlighted in pioneering studies (Jin, 1997a;Wyrtki, 1985), can precede ENSO SST anomalies up to five to seven seasons (Ballester et al., 2016;Izumo et al., 2019;Meinen & McPhaden, 2000), hence it has been argued recently as a better ENSO predictor beyond 1-yr lead times (Izumo et al., 2019;Planton et al., 2018). The slowly evolving heat content governed by the deterministic wind-driven ocean dynamics (Sverdrup transport) is presumably responsible for long-lead predictability of ENSO in climate models (Chen et al., 2004;Latif et al., 1998).