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1 1 Discrepant effects of atmospheric adjustments in shaping the spatial pattern of 1 SST anomalies between extreme and moderate El Niños 2 Jun Ying 1,2,3* , Tao Lian 1,4,3 , Ping Huang 5,2 , Gang Huang 2,6 , Dake Chen 1,4,3 and 3 Shangfeng Chen 5 4 1. State Key Laboratory of Satellite Ocean Environment Dynamics, Second Institute 5 of Oceanography, Ministry of Natural Resources, Hangzhou, 310012, China 6 2. State Key Laboratory of Numerical Modeling for Atmospheric Sciences and 7 Geophysical Fluid Dynamics, Institute of Atmospheric Physics, Chinese Academy 8 of Sciences, Beijing, 100190, China 9 3. Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), 10 Zhuhai, China 11 4. School of Oceanography, Shanghai Jiao Tong University, Shanghai, China 12 5. Center for Monsoon System Research, Institute of Atmospheric Physics, Chinese 13 Academy of Sciences, Beijing 100190, China 14 6. University of Chinese Academy of Sciences, Beijing, 100049, China 15 *Corresponding to: Dr. Jun Ying, email: [email protected],cn 16 17 Early Online Release: This preliminary version has been accepted for publication in Journal of Climate, may be fully cited, and has been assigned DOI he final typeset copyedited article will replace the EOR at the above DOI when it is published. © 20 ological Society T 21 American Meteor 10.1175/JCLI-D-20-0757.1. Brought to you by INSTITUTE OF ATMOSPHERIC PHYSICS, CAS | Unauthenticated | Downloaded 04/02/21 02:42 AM UTC
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1

Discrepant effects of atmospheric adjustments in shaping the spatial pattern of 1

SST anomalies between extreme and moderate El Niños 2

Jun Ying1,2,3*, Tao Lian1,4,3, Ping Huang5,2, Gang Huang2,6, Dake Chen1,4,3 and 3

Shangfeng Chen5 4

1. State Key Laboratory of Satellite Ocean Environment Dynamics, Second Institute 5

of Oceanography, Ministry of Natural Resources, Hangzhou, 310012, China 6

2. State Key Laboratory of Numerical Modeling for Atmospheric Sciences and 7

Geophysical Fluid Dynamics, Institute of Atmospheric Physics, Chinese Academy 8

of Sciences, Beijing, 100190, China 9

3. Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), 10

Zhuhai, China 11

4. School of Oceanography, Shanghai Jiao Tong University, Shanghai, China 12

5. Center for Monsoon System Research, Institute of Atmospheric Physics, Chinese 13

Academy of Sciences, Beijing 100190, China 14

6. University of Chinese Academy of Sciences, Beijing, 100049, China 15

*Corresponding to: Dr. Jun Ying, email: [email protected],cn 16

17

Early Online Release: This preliminary version has been accepted for publication in Journal of Climate, may be fully cited, and has been assigned DOI he final typeset copyedited article will replace the EOR at the above DOI when it is published. © 20 ological Society

T

21 American Meteor

10.1175/JCLI-D-20-0757.1.

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Abstract 18

The surface heat flux anomalies during El Niño events have always been treated 19

as an atmospheric response to sea surface temperature anomalies (SSTAs). However, 20

whether they play roles in the formation of SSTAs remain unclear. In this study, we 21

find that the surface net heat flux anomalies in different El Niño types have different 22

effects on the development of the spatial pattern of SSTAs. By applying the fuzzy 23

clustering method, El Niño events during 1982–2018 are classified into two types: 24

extreme (moderate) El Niños with strong (moderate) positive SSTAs, with the largest 25

SSTAs in the eastern (central) equatorial Pacific. The surface net heat flux anomalies 26

in extreme El Niños generally display a “larger warming gets more damping” zonal 27

paradigm, and essentially do not impact the formation of the spatial pattern of SSTAs. 28

Those in moderate El Niños, however, can impact the formation of the spatial pattern 29

of SSTA, by producing more damping effects in the eastern than in the central 30

equatorial Pacific, thus favoring the largest SSTAs being confined to the central 31

equatorial Pacific. The more damping effects of net heat flux anomalies in the eastern 32

equatorial Pacific in moderate El Niños are contributed by the surface latent heat flux 33

anomalies, which are mainly regulated by the negative relative humidity–SST 34

feedback and the positive wind–evaporation–SST feedback. Therefore, we highlight 35

that these two atmospheric adjustments should be considered during the development 36

of moderate El Niños in order to obtain a comprehensive understanding of the 37

formation of El Niño diversity. 38

Key words: extreme El Niño, moderate El Niño, latent heat flux anomalies, relative 39

humidity–SST feedback, wind–evaporation–SST feedback 40

Accepted for publication in Journal of Climate. DOI 10.1175/JCLI-D-20-0757.1.Brought to you by INSTITUTE OF ATMOSPHERIC PHYSICS, CAS | Unauthenticated | Downloaded 04/02/21 02:42 AM UTC

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1. Introduction 41

El Niño events are characterized by anomalous warm sea surface temperature 42

(SST) in the central-eastern equatorial Pacific, which have severe impacts on global 43

climate and human society (Barsugli et al. 1999; Wu et al. 2004; McPhaden et al. 44

2006; Cai et al. 2015; Timmermann et al. 2018). In recent decades, extensive studies 45

have revealed that El Niño events differ in terms of temporal evolution (Lengaigne 46

and Vecchi 2010; Xie et al. 2018), amplitude (Chen et al. 2016; Cai et al. 2017), and 47

spatial pattern (Ashok et al. 2007; Kao and Yu 2009; Kug et al. 2009; Chen et al. 48

2015). These differences give El Niño its different “flavors” and lead to different 49

climate impacts (Alexander et al. 2002; An et al. 2007; Kim et al. 2009; Yuan and 50

Yang 2012). In particular, the different spatial patterns of El Niño, generally measured 51

by the different zonal locations of the largest SST anomalies (SSTAs), can induce 52

distinct climate anomalies worldwide through air–sea interaction processes and 53

atmospheric teleconnections (Horel and Wallace 1981; Larkin and Harrison 2005; 54

Taschetto and England 2009; Taschetto et al. 2016; Xu et al. 2019). Understanding the 55

diversity of spatial pattern of El Niño and its formation mechanisms are crucial for a 56

reliable prediction of El Niño, as well as the associated climate and socioeconomic 57

impacts (Capotondi et al. 2015). 58

One notable manifestation of the diversity of spatial pattern of El Niño is that 59

most El Niño events present moderately warm SSTAs with the largest magnitude in 60

the central Pacific, while a few extreme El Niños have extraordinarily warm SSTAs 61

that are centered in the equatorial eastern Pacific close to the South American coast 62

(Takahashi et al. 2011). Much attention has been paid to the differences in the 63

formation mechanisms between extreme and moderate El Niños (Jin et al. 2003; Chen 64

et al. 2015; Chen et al. 2016). For instance, oceanic nonlinear dynamic heating was 65

Accepted for publication in Journal of Climate. DOI 10.1175/JCLI-D-20-0757.1.Brought to you by INSTITUTE OF ATMOSPHERIC PHYSICS, CAS | Unauthenticated | Downloaded 04/02/21 02:42 AM UTC

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revealed to be an essential role for developing extreme El Niños (Jin et al. 2003); 66

oceanic vertical advection anomalies caused by thermocline deepening are believed to 67

be the dominant contributor for extreme El Niños, but not for moderate ones (Kug et 68

al. 2009; Chen et al. 2015); and zonal advection anomalies caused by anomalous 69

zonal currents appear to be the most important factor contributing to the discrepant 70

magnitudes of SSTAs in the eastern Pacific between extreme and non-extreme El 71

Niños (Chen et al. 2016). However, these studies mainly concentrated on the role of 72

dynamic ocean heat transport, with little attention on the discrepant effects of 73

atmospheric adjustments on the development of SSTAs between extreme and 74

moderate El Niños. 75

In general, atmospheric adjustments during the development of El Niño SSTAs 76

are always treated as damping roles to balance the positive effects from dynamic 77

ocean heat transport anomalies, as they produce negative surface heat flux anomalies 78

(Jin et al. 2006; Zhang and McPhaden 2008; Chen et al. 2015; Chen et al. 2016; Lian 79

et al. 2017). However, it has been revealed that the spatial patterns of surface heat flux 80

anomalies do not always exhibit a straightforward reversed relationship with the 81

pattern of SSTAs (Wang and McPhaden 2000; Pavlakis et al. 2008). For example, the 82

surface latent heat flux anomalies near and to the west of the dateline were revealed to 83

play a positive role in the development of locally warm SSTAs owing to reduced 84

surface wind speed (Wang and McPhaden 2000); and the largest negative shortwave 85

radiation anomalies during El Niño events are usually found to be located to the west 86

of the positive SSTA center as a result of more convective activities locally (Pavlakis 87

et al. 2008; Pinker et al. 2017). These findings imply that atmospheric adjustments 88

may not only act in damping roles, but could also impact the spatial pattern of El Niño 89

SSTAs. 90

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There are considerable differences in the atmospheric responses to warm SSTAs 91

between extreme and moderate El Niños. For example, the Intertropical Convergence 92

Zone, whose climatological position is north of the equator, migrates towards the 93

eastern equatorial Pacific and turns the normally dry cold tongue condition into heavy 94

rainfall under an extreme El Niño, but maintains north of the equator under a 95

moderate El Niño and keeps the rainfall anomalies in the eastern equatorial Pacific 96

small (Cai et al. 2014; Cai et al. 2017; Hu and Fedorov 2018); and the westerly 97

anomalies induced by convective heating intrude into the eastern Pacific during an 98

extreme El Niño, but are confined to the central-western Pacific during a moderate 99

one (Lengaigne and Vecchi 2010; Xie et al. 2018; Peng et al. 2020). These different 100

responses imply discrepant atmospheric adjustments between extreme and moderate 101

El Niños, which may in turn lead to discrepant effects on the further development of 102

SSTAs through coupled ocean–atmosphere interaction processes (Bjerknes 1969; Xie 103

and Philander 1994). However, it is still unclear whether atmospheric adjustments 104

play different roles in the developing phase of SSTAs between extreme and moderate 105

El Niños. Moreover, whether atmospheric adjustments impact the formation of the 106

spatial pattern of El Niño SSTAs, rather than merely acting in damping roles, also 107

needs to be further explored. 108

In this study, we investigate the discrepant effects of atmospheric adjustments on 109

the spatial pattern formations of SSTAs during the developing phase of extreme and 110

moderate El Niños, as well as the underlying mechanisms. We find that surface net 111

heat flux anomalies in extreme El Niños, generally displaying a “larger warming gets 112

more damping” zonal paradigm, have little impact on the formation of the zonal 113

pattern of SSTAs, while those in moderate El Niños can help shape the zonal pattern 114

of SSTAs by producing more damping effects in the eastern than central equatorial 115

Accepted for publication in Journal of Climate. DOI 10.1175/JCLI-D-20-0757.1.Brought to you by INSTITUTE OF ATMOSPHERIC PHYSICS, CAS | Unauthenticated | Downloaded 04/02/21 02:42 AM UTC

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Pacific, thus favoring larger SSTAs being located in the central equatorial Pacific. 116

The rest of the paper is organized as follows: Section 2 describes the data and 117

methods used in the study. Section 3 presents the main results, including the objective 118

separation of extreme El Niños from other moderate ones, the discrepant effects of 119

surface net heat flux anomalies during the developing phase between extreme and 120

moderate El Niños and the associated formation mechanisms. Conclusions and 121

discussion are given in Section 4. 122

2. Data and methods 123

2.1 Datasets 124

The monthly SST data are from the National Oceanic and Atmospheric 125

Administration (NOAA) Optimum Interpolation SST, version 2, with a horizontal grid 126

resolution of 1° × 1°, which is provided by the NOAA Earth Research Laboratory 127

Physical Science Division (http://www.esrl.noaa.gov/psd/data). The monthly 128

atmospheric data are from the fifth major global reanalysis developed by the 129

European Centre for Medium-Range Weather Forecasts (ERA5, 130

https://cds.climate.copernicus.eu/cdsapp#!/dataset/reanalysis-era5-single-levels-month131

ly-means?tab=form), with a horizontal resolution of 0.25° × 0.25°, including the 132

surface latent heat flux, sensible heat flux, net shortwave radiation, net longwave 133

radiation, precipitation, boundary-layer height, surface zonal and meridional winds, 134

surface wind speed, air temperature, and three-dimensional relative humidity. Besides, 135

the monthly SST from ERA5 is chosen only for computing the regressions between 136

SSTAs and relative humidity anomalies, and between SSTAs and boundary-layer 137

height anomalies. The monthly oceanic three-dimensional data are from the National 138

Centers for Environmental Prediction (NCEP) Global Ocean Data Assimilation 139

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System (GODAS, https://www.esrl.noaa.gov/psd/data/gridded/data.godas.html), with 140

a horizontal resolution of 1/3° longitude × 1° latitude. In addition, we also use surface 141

net heat fluxes from GODAS and the NCEP–National Center for Atmospheric 142

Research (NCAR) reanalysis 143

(https://psl.noaa.gov/data/gridded/data.ncep.reanalysis.html) to confirm the results 144

derived from ERA5. All the datasets are chosen for the period 1982–2018 during 145

which all variables are available. The monthly anomalies are obtained by removing 146

the long-term trend as well as the climatological annual cycle of the chosen time 147

period, and then a three-month running mean is applied to reduce the intraseasonal 148

variability. 149

2.2 Fuzzy clustering method 150

The fuzzy clustering method (FCM), which has been proved to be an effective 151

pattern-classification technique in climate research (Kim et al. 2011; Chen et al. 2015), 152

is used to classify different El Niño types in this study. Unlike some other El Niño 153

classification techniques that rely on prior knowledge of different El Niño patterns 154

(Kao and Yu 2009; Kug et al. 2009), the FCM doesn’t need to presume the different 155

patterns of El Niño ahead of time, while leaving the data to be self-clustering 156

objectively (Feng et al. 2020). It is designed to group a set of given members into 157

specified categories based on their degree of membership (DOM), which stands for 158

the similarity of members to the centroids. The DOM is defined as the 159

root-mean-squared Euclidean distance to the cluster center and can be expressed as 160

M N2 2 2

i,j j ii 1 j=1min( ( ) )e P X C

, (1) 161

where 162

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12

2

M j i

i,j 2k=1

j k

X CP a

X C

, (2) 163

and 164

N 2

i,j jj=1

i N 2

i,jj=1

P XC

P

. (3) 165

Here, N is the size of members, M is the number of cluster sets, jX is the map of 166

the member, iC is the map of the ith cluster centroid,

i,jP is the DOM of jX to

iC , 167

the symbol denotes Euclidean distance, and a is a scale factor to guarantee that 168

M

i,ji 11P

for j=1 to N . 169

The members applied to the FCM here are a subset of the monthly SSTAs in the 170

tropical Pacific (150°E–90°W, 20°S–20°N) during El Niño events. We first use a 40° 171

× 10° window zonally sliding by 2.5° along the equator (5°S–5°N), starting from 172

150°E to 90°W, in order to obtain a set of regional mean SSTAs and the 173

corresponding standard deviations (STDs). The month in which any regional-mean 174

SSTA is greater than the corresponding positive STD and 0.5℃ is then regarded as a 175

warm record. When all the warm records are extracted, those segments with less than 176

five successive months in the set of warm records are deleted. Moreover, as the peak 177

time of El Niño tends to be phase locked in boreal winter (Tziperman et al. 1998), the 178

warm segments that do not contain boreal winter time (November–January) are also 179

discarded. The remaining warm months are then used for our classification of 180

different El Niño types. In addition, the type of a specific El Niño event is based on 181

the type into which its DOM in boreal winter falls. Details regarding the application 182

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of the FCM technique in El Niño classification can also be found in Chen et al. 183

(2015). 184

2.3 Ocean mixed-layer heat budget analysis 185

Following Ying et al. (2016), the mixed-layer temperature tendency equation can 186

be simplified as 187

Ou v w net res

TC Q Q Q Q Q

t

, (4) 188

where the prime denotes the monthly anomaly; OT is the ocean mixed-layer 189

temperature anomaly; p oC C H is the heat capacity of the ocean mixed-layer; 190

1

p 4000C J kg K and 3

o =1025kg m are the specific heat at constant pressure 191

and density of seawater, respectively; H is the mixed-layer depth, which is chosen 192

as a constant of 30 m for simplicity, as in (Ying et al. 2016); u ( / )Q C uo T x , 193

v = ( / )Q C vo T y and w ( / )Q C wo T z are the ocean zonal, meridional and 194

vertical heat transport anomalies in the mixed-layer, respectively, uo , vo , and wo 195

are the ocean zonal, meridional and vertical current averaged in the mixed-layer; netQ 196

is the surface net heat flux anomalies (positive downward), including the anomalous 197

surface latent heat flux ( EQ ), sensible heat flux ( HQ ), net longwave radiation ( LWQ ), 198

and net shortwave radiation (SWQ ); resQ is the residual term, including anomalies in 199

the ocean sub-grid scale processes such as vertical mixing and lateral entrainment 200

(DiNezio et al. 2009; Ying et al. 2016). 201

2.4 Decomposition of the surface latent heat flux anomaly 202

Among the surface heat fluxes, the latent heat flux plays a critical role in 203

modulating SST variations (Wang and McPhaden 2000; Xie et al. 2010; Jia and Wu 204

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2013), which can be calculated by the following bulk formula: 205

E a E s s( )(1 )TQ LC Wq T RHe , (5) 206

where a is surface air density; L is the latent heat of evaporation;

EC is the 207

exchange coefficient; W is the surface wind speed at 10 m; s s( )q T is the saturated 208

specific humidity; RH is the surface relative humidity; sT is SST, and a s=T T T 209

is the difference between the surface air temperature (aT ) and SST, denoting the 210

surface stability; and 2 1

v s/ ( ) 0.06 KL R T , in which vR is the ideal gas 211

constant for water vapor. To estimate the contributions of each factor during the 212

development of El Niño, the EQ is decomposed following previous studies (Du and 213

Xie 2008; Xie et al. 2010; Jia and Wu 2013): 214

E E E EE s

s

=Q Q Q Q

Q T W RH TT W RH T

. (6) 215

Each term on the right-hand-side of Eq. (6) can be expressed as follows: 216

EEO s E s

s

QQ T Q T

T

; (7) 217

E EEW

Q QQ W W

W W

; (8) 218

E EERH T

Q QQ RH RH

RH e RH

; (9) 219

E EE T T

Q Q RHQ T T

T e RH

. (10) 220

Here, an overbar and prime denote the monthly climatology and anomaly, respectively. 221

Equation (7) represents the Newtonian cooling effect in response to SSTAs, while Eqs. 222

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(8)–(10) represent the atmospheric adjustments due to anomalies in surface wind 223

speed, relative humidity and surface stability, respectively. Specifically, the EWQ is 224

commonly known as the wind–evaporation–SST (WES) feedback (Xie and Philander 225

1994), which can be further decomposed into effects from surface zonal and 226

meridional wind anomalies: 227

EEu 2

Q uQ u

W (11) 228

and 229

EEv 2

Q vQ v

W , (12) 230

where u and v denote the surface zonal and meridional wind, respectively. 231

3. Results 232

3.1 Classification of El Niños based on the FCM 233

The FCM is applied to classify El Niño events during 1982–2018 into two types. 234

As shown in Fig. 1, the first warm pattern displays robust positive SSTAs in the 235

central and eastern Pacific and has its largest warming in the eastern equatorial Pacific 236

near the South American coast (Fig. 1a), which is a typical feature of extreme El 237

Niños (Takahashi et al. 2011; Chen et al. 2015; Xie et al. 2018). Three historical El 238

Niños, commonly known as the extreme El Niño events of 1982/83, 1997/98 and 239

2015/16 (Cai et al. 2017; Lian et al. 2017), fall into the first pattern classification (Fig. 240

1c, red curve). The second warm pattern exhibits moderately positive SSTAs centered 241

in the central equatorial Pacific east of the dateline around 170°W (Fig. 1b). Nine 242

historical El Niños other than the three aforementioned extreme ones—in 1986/87, 243

1987/88, 1991/92, 1994/95, 2002/03, 2004/05, 2006/07, 2009/10 and 2014/15—are 244

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all classified as the second warm pattern (Fig. 1c, blue curve). Thus, the FCM 245

naturally separates the extreme El Niños from other moderate El Niños when two 246

clusters are set. Moreover, the classified result by the FCM indicates that the pattern 247

differences between extreme and moderate El Niños appear to be the most robust 248

among different El Niño types. 249

3.2 Discrepant roles of net

Q for the development of SSTA patterns between 250

extreme and moderate El Niños 251

Figure 2 presents the spatial patterns of SSTAs, SSTA tendencies and netQ 252

during developing phase (from May to December of the developing year) of the 253

extreme and moderate El Niños. It is shown that the largest SSTAs during the 254

developing phase appear to be anchored basically in the eastern equatorial Pacific east 255

of 150°W in extreme El Niños (Fig. 2a), while those in moderate El Niños are mostly 256

confined to the central Pacific around 150°–170°W (Fig. 2c). Such a difference is 257

consistent with the different warm patterns classified by the FCM (Figs. 1a and b). 258

Moreover, the SSTA tendencies during the developing phase display similar zonal 259

patterns to the corresponding SSTAs, with more positive values in the eastern (central) 260

than in the central (eastern) equatorial Pacific in extreme (moderate) El Niños (Figs. 261

2b and d, contours). On the other hand, the damping effects of netQ in extreme and 262

moderate El Niños are both larger in the eastern equatorial Pacific east of 140°W, 263

albeit with a larger amplitude for the extreme ones (Figs. 2b and d). The former 264

matches well with the corresponding gradual increases of positive SSTAs from the 265

central to the eastern equatorial Pacific (Fig. 2e, solid curves), thus generally 266

displaying a “larger warming gets more damping” zonal paradigm, while the latter 267

zonally deviates from the corresponding larger positive SSTAs in the central 268

equatorial Pacific west of 140°W (Fig. 2e, dashed curves). Accordingly, in moderate 269

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El Niños, the more damping effects of netQ and the weaker positive SSTA tendencies, 270

both in the eastern equatorial Pacific, imply that the damping effect of netQ may help 271

contribute to the local weaker SSTA tendencies, favoring larger SSTA tendencies as 272

well as larger SSTAs being located in the central equatorial Pacific (Fig. 2d). Similar 273

results can be found based on the netQ from the GODAS and NCEP–NCAR datasets 274

(Fig. 3). In these two datasets, the larger damping effects of netQ in extreme El 275

Niños generally match well with the larger SSTA tendencies (Figs. 3a and b), while 276

those in moderate El Niños zonally deviate from the larger SSTA tendencies (Figs. 3c 277

and d). 278

With regards to each individual El Niño event, it is shown that all the three 279

extreme El Niños exhibit larger positive (negative) SSTAs (netQ ) in the eastern than 280

central equatorial Pacific, and most of the moderate El Niños display larger positive 281

SSTAs (negative netQ ) in the central (eastern) than eastern (central) equatorial Pacific, 282

leading to the average of positive SSTAs (negative netQ ) in moderate El Niños being 283

larger in the central (eastern) equatorial Pacific (Fig. 4). Note that the 94/95 El Niño 284

event is an outlier of moderate El Niño with larger negative netQ in the central 285

equatorial Pacific. In addition, there are slightly larger positive SSTAs but much 286

larger negative netQ in the eastern equatorial Pacific for the 87/88, 09/10 and 14/15 287

El Niño events. These outliers imply that there could be an intermediate state of SSTA 288

pattern with no explicit difference between central and eastern Pacific warm 289

anomalies (Chen et al. 2015). Nevertheless, they are classified into moderate El Niños 290

as the zonal SSTA patterns of these three El Niños are more close to the second type 291

based on the FCM (Fig. 1b). In the following section, we will reveal that the effects of 292

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netQ on the zonal SSTA pattern formations for these outliers are physically consistent 293

with the common moderate El Niños. 294

Figure 5 displays a Hovmöller diagram (averaged over 2.5°S–2.5°N) that 295

compares the temporal evolutions of equatorial SSTAs as well as netQ during the 296

developing year between extreme and moderate El Niño events. Extreme and 297

moderate El Niños both present warm SSTAs firstly in the central equatorial Pacific in 298

early spring of the developing year, and follow discrepant developing trajectories of 299

the zonal SSTA pattern afterwards. In extreme El Niños, the largest SSTAs appear to 300

be anchored basically in the eastern equatorial Pacific east of 150°W after May of the 301

developing year (Fig. 5a), while those in moderate El Niños are mostly confined to 302

the central Pacific around 150°–170°W (Fig. 5c). Such a difference is consistent with 303

the different SSTA patterns averaged over the developing phase (Figs. 2a and c). 304

Meanwhile, the SSTA tendencies during the developing phase show overall similar 305

zonal distributions to the corresponding SSTAs, with more positive values in the 306

eastern (central) than central (eastern) equatorial Pacific in extreme (moderate) El 307

Niños (Figs. 5a and c, contours). On the other hand, the more damping effects of netQ 308

in extreme and moderate El Niños are both located in the eastern equatorial Pacific 309

during the developing phase (Figs. 5b and d). The former matches well with the 310

corresponding zonal pattern of SSTAs, while the latter is anchored in the eastern 311

equatorial Pacific and zonally deviates from the corresponding more positive SSTAs 312

in the central equatorial Pacific. 313

To quantify the discrepant effects of netQ on the development of zonal SSTA 314

patterns between extreme and moderate El Niño, an ocean mixed-layer heat budget 315

analysis is further conducted based on the GODAS dataset (Fig. 6) during the 316

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developing phase of the two El Niño clusters both in the eastern (2.5°S–2.5N, 317

140°W–90°W; red bars) and central equatorial Pacific (2.5°S–2.5N, 180°–140°W; 318

blue bars), together with their differences (black bars). Note that the spatial patterns of 319

the chosen mixed-layer temperature anomalies are quite similar to those of the SSTAs 320

both in extreme and moderate El Niños (not shown). Concurrent with the SSTA 321

tendencies (Figs. 2b and d, contours), the ocean mixed-layer temperature tendencies 322

(O /C T t ) for extreme El Niños are larger in the eastern than central equatorial 323

Pacific (Fig. 6a). Such zonal distribution is contributed by the ocean 324

three-dimensional heat transport anomalies, among which the wQ contributes the 325

most, consistent with previous studies (Kug et al. 2009; Chen et al. 2015). While the 326

netQ , acting as the major damping term, displays a much more damping effect in the 327

eastern than in the central equatorial Pacific. This indicates that the damping effect of 328

netQ could not essentially alter the zonal distribution of O /C T t owing to the 329

overwhelming positive effect from ocean heat transport anomalies, but merely to be a 330

response to positive SSTAs. 331

By contrast, the O /C T t in the central equatorial Pacific are a little bit larger 332

than that in the eastern equatorial Pacific for moderate El Niños (Fig. 6b). Similar to 333

the extreme El Niños, the contribution of ocean three-dimensional heat transport 334

anomalies in moderate El Niños, albeit with a much smaller magnitude, also favors 335

more positive SSTAs in the eastern than in the central Pacific, while the netQ acts to 336

suppress such effect. This indicates that the more damping effects of netQ in the 337

eastern equatorial Pacific might alter the zonal distribution of O /C T t in moderate 338

El Niños by partly offsetting the local modest positive effects of ocean heat transport 339

anomalies, favoring more positive SSTAs to be located in the central equatorial 340

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Pacific. 341

The resQ in extreme El Niños is negligible but appears to be another contributor 342

to the zonal SSTA pattern formation in moderate El Niños by producing negative 343

(positive) effects in the eastern (central) Pacific, favoring more positive SSTAs in the 344

central equatorial Pacific. Thus, the role of oceanic sub-grid scale processes, which 345

are beyond the scope of this study, should be paid more attention to in shaping the 346

zonal SSTA pattern of moderate El Niños. 347

3.3 Discrepant atmospheric adjustments involved in net

Q between extreme and 348

moderate El Niños 349

Figure 7 displays the spatial patterns of SWQ , EQ , and the sum of both in the 350

developing phase for the two types of El Niño. It is shown that the sum of EQ and 351

SWQ matches well with the spatial patterns of netQ , both in extreme and moderate El 352

Niños, with the spatial correlations both exceeding 0.98 (Figs. 7c and f). This 353

indicates that the EQ and SWQ dominate the netQ , while the HQ and LWQ (not 354

shown) are negligible. The negative SWQ , with their damping centers being located in 355

the central equatorial Pacific in response to the atmospheric deep convection 356

anomalies, extends to the eastern equatorial Pacific in extreme El Niños (Fig. 7a), but 357

are confined to the central equatorial Pacific west of 180° and the north of the eastern 358

Pacific in moderate El Niños (Fig. 7d). The EQ exhibits a zonal dipole pattern both 359

in extreme and moderate El Niños, with weak (strong) positive (negative) anomalies 360

in the central (eastern) equatorial Pacific (Figs. 7b and e). The sum of SWQ and EQ 361

shows that the positive effects of EQ in the central equatorial Pacific are totally 362

offset by the local negative effects of SWQ , and the negative effects of EQ dominate 363

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the damping role of netQ in the eastern equatorial Pacific, leading to relatively weak 364

damping effects in the central equatorial Pacific and strong damping effects in the 365

eastern equatorial Pacific, both in extreme and moderate El Niños (Figs. 7c and f). 366

Therefore, the EQ plays a dominant role both in the “larger warming gets more 367

damping” zonal paradigm of netQ in extreme El Niños and in the zonal deviation 368

between the positive SSTA center and the negative netQ center in moderate El Niños. 369

The factors contributing to EQ are further compared between extreme and 370

moderate El Niños (Fig. 8). The reconstructed spatial patterns and magnitudes of EQ 371

in extreme and moderate El Niños are almost identical compared with their original 372

counterparts (Figs. 7b and e), with the spatial correlations both exceeding 0.97, 373

indicating that the decomposition of EQ based on Eq. (6) is reasonable. The oceanic 374

response represented by EOQ plays a negative role both in extreme and moderate El 375

Niños (Figs. 8b and g). Regarding the atmospheric adjustments, the EWQ is totally 376

negative in the eastern equatorial Pacific in moderate El Niños, but involves both 377

positive and negative effects in extreme El Niños (Figs. 8c and h); the ERHQ appears 378

to play a critical role in the damping effects of EQ in the eastern equatorial Pacific 379

both in extreme and moderate El Niños (Figs. 8d and i); and the E TQ plays another 380

important role for the damping effects in the eastern equatorial Pacific in extreme El 381

Niños with local robust positive SSTAs, but is negligible in moderate El Niños with 382

weak SSTAs (Figs.8e and j). 383

The discrepant effects of EWQ in the eastern equatorial Pacific between extreme 384

and moderate El Niños could be due to local different positive WES feedback 385

processes. In extreme El Niños, the robust positive SSTAs in the eastern equatorial 386

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Pacific trigger local deep convections (Fig. 7a, contours). The convective heating 387

causes surface convergent anomalies in the eastern equatorial Pacific, including the 388

intrusion of strong westerly wind anomalies from the central to the eastern equatorial 389

Pacific (Fig. 9a; Xie et al., 2018) and the convergence of meridional wind anomalies 390

to the equator (Fig. 9b). The intrusion of westerly anomalies weakens the background 391

easterly winds and lowers the surface evaporation, contributing positively to the 392

growth of warm SSTAs in the eastern equatorial Pacific (Fig. 9a), while the 393

convergence of meridional wind anomalies weakens (enhances) the background 394

cross-equatorial southerly winds and increases (decreases) the SSTAs north (south) of 395

the equator (Fig. 9b). The positive and negative effects of EWQ largely 396

counterbalance each other in the eastern equatorial Pacific, leading to relatively small 397

negative effects on the growth of SSTAs (Fig. 8c). In moderate El Niños, however, the 398

relatively weak positive SSTAs in the eastern Pacific cannot trigger local deep 399

convections due to too cold background SST, but could be sufficient enough to trigger 400

deep convections in the central equatorial Pacific and the climatological ITCZ region 401

north of the eastern Pacific where the background SSTs are already high (Fig. 7d, 402

contours), thus causing westerly anomalies confined to the central-western Pacific and 403

cross-equatorial southeasterly anomalies in the eastern equatorial Pacific (Figs. 9c and 404

d). The SSTA-induced southeasterly anomalies can feed back to the further 405

development of SSTAs by enhancing the background southeasterlies and evaporation 406

through the WES feedback, which produce prominent damping effects on the 407

subsequent growth of SSTAs in the eastern equatorial Pacific and favor larger SSTAs 408

to be located in the central equatorial Pacific. 409

The damping effects of ERHQ in the eastern equatorial Pacific could be 410

attributable to the local negative feedback between SST and relative humidity. To 411

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verify such feedback, we define a relative humidity–SST feedback index (RSFI) by 412

regressing the monthly anomalies of surface relative humidity onto the SSTAs. As 413

shown in Fig. 10a, prominent negative RSFI values appear in the eastern equatorial 414

Pacific. This indicates that the positive SSTAs in the eastern equatorial Pacific during 415

El Niño events will reduce the local relative humidity, which further suppresses the 416

growth of local SSTAs by inducing negative EQ (Figs. 8d and i). Such inherent 417

negative feedback could be due to local strong vertical mixing between the 418

boundary-layer with relative high relatively humidity and the upper free atmosphere 419

with relatively low relative humidity (Fig. 10c, contours) that is induced by positive 420

SSTAs. The positive SSTAs increase the production of vertical mixing in the eastern 421

Pacific boundary layer where the stratocumulus prevails (Wood 2012), thus enhancing 422

the entrainment of upper-level dry air at the stratus cloud top, which tends to desiccate 423

the whole boundary layer (Scott et al. 2020) and raise the boundary layer height. 424

Indeed, the equatorial RSFIs are negative from the surface to the top of the boundary 425

layer (which is also the stratus cloud top) where the climatological relative humidity is 426

the largest due to the vertical mixing, but are positive in the upper free atmosphere 427

(Fig. 10c, shaded). Moreover, there are positive feedbacks between the monthly 428

anomalies of boundary-layer height and SST in the eastern equatorial Pacific (BHFI, 429

Fig. 10b), further verifying a stronger vertical mixing between the boundary layer and 430

the free atmosphere that helps to reduce the surface relative humidity during El Niño 431

events (Deser and Wallace 1990; Ham et al. 2018). Therefore, no matter which type of 432

El Niño occurs, the inherent negative relative humidity–SST feedback helps to 433

confine the damping effects of EQ to the eastern equatorial Pacific, contributing to 434

both the “larger warming gets more damping” zonal paradigm in extreme El Niños 435

and the more SSTAs in the central equatorial Pacific in moderate El Niños. 436

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Figure 11 quantifies the major flux anomalies during the developing phase of El 437

Niño both in the eastern (2.5°S–2.5N, 140°–90°W) and central (2.5°S–2.5N, 438

180°–140°W) equatorial Pacific, as well as their differences. In extreme El Niños with 439

the larger SSTAs in the eastern equatorial Pacific, the netQ is mainly contributed by 440

both the SWQ and

EQ . The former contributes more damping effects in the central 441

equatorial Pacific, which are partly offset by the local positive effects of EWQ 442

involved in EQ , while the latter plays a dominant damping role in the eastern 443

equatorial Pacific, which is mainly contributed by EOQ ,

ERHQ , and E TQ . In 444

moderate El Niños with the larger SSTAs in the central equatorial Pacific, the zonal 445

deviation between the positive SSTA center and the negative netQ center is mainly 446

caused by more damping effects of EQ in the eastern equatorial Pacific, which are 447

mainly contributed by EOQ ,

EWQ , and ERHQ . Thus, apart from the oceanic response 448

(EOQ ), it appears that the positive WES feedback and the negative relative 449

humidity–SST feedback in the eastern equatorial Pacific are the two major 450

atmospheric adjustments that lead to the zonal deviation between the positive SSTA 451

center in the central Pacific and the negative netQ center in the eastern Pacific, 452

favoring the largest SSTAs being confined to the central equatorial Pacific in 453

moderate El Niños. 454

4. Conclusions and discussions 455

In this study, we reveal that the surface net heat flux anomalies ( netQ ), once 456

commonly regarded as responses to SSTAs in El Niño events, can play different roles 457

in the formation of SSTA patterns in different El Niño types. By applying the FCM, 458

the El Niño events during the period 1982–2018 are classified into two types: extreme 459

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El Niños and moderate El Niños. The former displays robust positive SSTAs and has 460

its largest SSTAs in the eastern equatorial Pacific, while the latter exhibits relatively 461

weak positive SSTAs and has its largest SSTAs in the central equatorial Pacific. It is 462

shown that the damping effects of netQ in the developing phase of extreme and 463

moderate El Niños are both larger in the eastern than in the central equatorial Pacific. 464

The former generally displays a “larger warming gets more damping” zonal paradigm 465

and essentially does not impact the spatial pattern of SSTA tendencies as well as the 466

pattern formation of SSTAs, while the latter can impact the spatial pattern formation 467

of SSTAs by damping the SSTA tendencies more in the eastern than in the central 468

equatorial Pacific, favoring the positive center of SSTAs being confined to the central 469

equatorial Pacific. An ocean mixed-layer heat budget analysis indicates that the 470

merely damping role of netQ in extreme El Niños could be attributable to the 471

overwhelming modulation of ocean heat transport anomalies, which play a decisive 472

role in the spatial pattern formation of SSTAs. Meanwhile, the netQ in moderate El 473

Niños could be a contributor to the SSTA pattern formation largely owing to the 474

modest modulation of ocean heat transport anomalies, leaving room for the damping 475

effects of netQ to function. 476

The netQ is mainly contributed by surface net shortwave radiation anomalies 477

and surface latent heat flux anomalies (EQ ), both in extreme and moderate El Niños, 478

among which the latter plays a dominant role. However, the atmospheric adjustments 479

involved in EQ play out differently between extreme and moderate El Niños. In 480

extreme El Niños, the negative relative humidity–SST feedback and the reduced 481

surface stability due to robust SSTAs are the two major atmospheric adjustments for 482

the damping effects of EQ in the eastern equatorial Pacific, while the WES feedback 483

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plays a negligible role owing to the counterbalance between the positive effects from 484

the eastward intrusion of the westerlies and the negative effects from the equatorial 485

convergence of meridional wind anomalies. 486

In moderate El Niños, the negative relative humidity–SST feedback also appears 487

to be the most dominant atmospheric adjustments for the damping effects of EQ in 488

the eastern equatorial Pacific, suggesting that the negative relative humidity–SST 489

feedback is an inherent regulator that helps to confine the damping effects of EQ to 490

the eastern equatorial Pacific regardless of the type of El Niño. In addition, the WES 491

feedback is revealed to be another major atmospheric adjustment for the damping 492

effects of EQ in the eastern equatorial Pacific, which is a result of local 493

cross-equatorial southeasterly anomalies caused by SSTA-induced deep convection 494

anomalies north of the eastern Pacific. Previous studies have revealed that the effects 495

of eastern Pacific wind anomalies are crucial for the discrepant decay trajectories 496

between extreme and moderate El Niño through different ocean dynamical heat 497

transports and WES feedback (Xie et al. 2018; Peng et al. 2020). Here we highlight 498

that the different wind anomalies during the developing phase also play roles in the 499

formation of different SSTA patterns between extreme and moderate El Niño owing to 500

the emergence of different SSTA-induced convective anomalies (Fig. 7a, d, contours). 501

Therefore, it is mainly the two atmospheric adjustments, the negative relative 502

humidity–SST feedback and the positive WES feedback, that favor the damping 503

effects of netQ to be more in the eastern than in the central equatorial Pacific and 504

contribute to more positive SSTAs in the central equatorial Pacific in moderate El 505

Niños. The former plays a dominant role, while the latter plays secondarily. 506

The classification of El Niño diversity has been always a heated debate in 507

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climate research community (Kao and Yu 2009; Takahashi et al. 2011; Karnauskas 508

2013; Chen et al. 2015). In a pioneering application of the FCM to the classification 509

of El Niño by Chen et al. (2015), three warm patterns are classified—the extreme El 510

Niños which is identical to the current first warm pattern, the warm-pool El Niños that 511

has weak positive SSTAs centered near the dateline and the canonical El Niños with 512

moderate positive SSTAs along the central-eastern equatorial Pacific. In this study, 513

however, we do not try to clarify different types of El Niño, but to explore different 514

atmospheric adjustments specifically between extreme and other non-extreme El 515

Niños. Therefore, the number of cluster set chosen here is two (i.e., M 2 in Eq. 1) 516

to highlight the different warm patterns between extreme El Niños and other moderate 517

ones. The main conclusions in this study do not change essentially between the 518

extreme El Niños and the other two non-extreme El Niños if three types of El Niño 519

are classified as in Chen et al. (2015). 520

The present study focuses on the discrepant effects of atmospheric adjustments 521

on the formation of zonal SSTA patterns in different El Niño types, with a particular 522

focus on contributions of atmospheric adjustments in the formation of SSTA patterns 523

in moderate El Niños, while the effects of ocean heat transport anomalies have not 524

been explored extensively. In fact, many studies have revealed that some specific 525

ocean dynamical processes play key roles in the development of SSTAs in specific El 526

Niño types (Kug et al. 2009; Chen et al. 2015; Lian et al. 2017). For instance, ocean 527

thermocline feedback was revealed to play the dominant role in the development of 528

extreme El Niños (Chen et al. 2015), while zonal advective feedback plays a crucial 529

role during warm pool El Niños (which essentially can be classified into moderate El 530

Niños in the current study) (Kug et al. 2009; Takahashi et al. 2011). Thus, the 531

atmospheric adjustment processes, especially for the relative humidity–SST feedback 532

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and the WES feedback in the eastern equatorial Pacific, could be supplementary 533

mechanisms in modulating the zonal pattern formation of SSTAs in moderate El 534

Niños, and do not conflict with previous ocean origin mechanisms. Moreover, these 535

atmospheric adjustments may play potential roles in predicting the SSTA pattern of El 536

Niño during the peak phase. For example, if the SSTA-induced deep convections do 537

not move to the eastern Pacific to trigger the conventional Bjerknes feedback during 538

the developing phase of an El Niño (Karnauskas 2013; Lian et al. 2017), the positive 539

SSTA center in the peak phase is likely to be more close to the central equatorial 540

Pacific, as the damping effects from atmospheric adjustments will further suppress the 541

growth of SSTAs in the eastern equatorial Pacific. They may also explain, to some 542

extent, why there are only few cases that have the spatial patterns similar to extreme 543

El Niño but with their magnitudes similar to moderate El Niño (McPhaden et al. 2011; 544

Zhang et al. 2015), though more details need to be provided to verify such 545

interpretation. We highlight that atmospheric adjustments should be considered during 546

the development of moderate El Niños in order to obtain a comprehensive 547

understanding of the formation of El Niño diversity. 548

549

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Acknowledgements 550

This work was supported by the Scientific Research Fund of the Second Institute of 551

Oceanography, Ministry of Natural Resources (Grant QNYC2001), the National 552

Natural Science Foundation of China (Grants 41690121, 41690120, 41706024, 553

41621064, 41831175), the Indo-Pacific Ocean Variability and Air-Sea Interaction 554

(IPOVAI, Grant GASI-01-WPAC-STspr), the Youth Innovation Promotion 555

Association of the Chinese Academy of Sciences and the Key Deployment Project of 556

Centre for Ocean Mega-Research of Science,Chinese Academy of Sciences (Grant 557

COMS2019Q03). We thank Prof. Jian Ma and Doc. Qun Liu for their helpful 558

discussions. 559

560

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Niño: Implications for ENSO Diversity. Journal of Climate, 33, 3197-3212. 645

Pinker, R. T., S. A. Grodsky, B. Zhang, A. J. Busalacchi, and W.-Y. Chen, 2017: 646

ENSO impact on surface radiative fluxes as observed from space. Journal of 647

Geophysical Research, 122, 7880-7896. 648

Scott, R. C., T. A. Myers, J. R. Norris, M. D. Zelinka, S. A. Klein, M. Sun, and D. R. 649

Accepted for publication in Journal of Climate. DOI 10.1175/JCLI-D-20-0757.1.Brought to you by INSTITUTE OF ATMOSPHERIC PHYSICS, CAS | Unauthenticated | Downloaded 04/02/21 02:42 AM UTC

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Doelling, 2020: Observed Sensitivity of Low-Cloud Radiative Effects to 650

Meteorological Perturbations over the Global Oceans. Journal of Climate, 33, 651

7717-7734. 652

Takahashi, K., A. Montecinos, K. Goubanova, and B. Dewitte, 2011: ENSO regimes: 653

Reinterpreting the canonical and Modoki El Niño. Geophysical Research 654

Letters, 38. 655

Taschetto, A. S., and M. H. England, 2009: El Niño Modoki Impacts on Australian 656

Rainfall. Journal of Climate, 22, 3167-3174. 657

Taschetto, A. S., R. R. Rodrigues, G. A. Meehl, S. McGregor, and M. H. England, 658

2016: How sensitive are the Pacific–tropical North Atlantic teleconnections to 659

the position and intensity of El Niño-related warming? Climate Dynamics, 46, 660

1841-1860. 661

Timmermann, A., and Coauthors, 2018: El Niño–Southern Oscillation complexity. 662

Nature, 559, 535-545. 663

Tziperman, E., M. A. Cane, S. E. Zebiak, Y. Xue, and B. Blumenthal, 1998: Locking 664

of El Niño’s Peak Time to the End of the Calendar Year in the Delayed 665

Oscillator Picture of ENSO. Journal of Climate, 11, 2191-2199. 666

Wang, W., and M. J. McPhaden, 2000: The Surface-Layer Heat Balance in the 667

Equatorial Pacific Ocean.Part II: Interannual Variability. Journal of Physical 668

Oceanography, 30, 2989-3008. 669

Wood, R., 2012: Stratocumulus Clouds. Monthly Weather Review, 140, 2373-2423. 670

Wu, M. C., W. L. Chang, and W. M. Leung, 2004: Impacts of El Niño–Southern 671

Oscillation Events on Tropical Cyclone Landfalling Activity in the Western 672

North Pacific. Journal of Climate, 17, 1419-1428. 673

Xie, S.-P., and S. G. H. Philander, 1994: A coupled ocean-atmosphere model of 674

relevance to the ITCZ in the eastern Pacific. Tellus 46, 340-350. 675

Xie, S.-P., C. Deser, G. A. Vecchi, J. Ma, H. Teng, and A. T. Wittenberg, 2010: Global 676

Warming Pattern Formation: Sea Surface Temperature and Rainfall. Journal of 677

Climate, 23, 966-986. 678

Xie, S.-P., Q. Peng, Y. Kamae, X.-T. Zheng, H. Tokinaga, and D. Wang, 2018: Eastern 679

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Pacific ITCZ Dipole and ENSO Diversity. Journal of Climate, 31, 4449-4462. 680

Xu, K., Q.-L. Huang, C.-Y. Tam, W. Wang, S. Chen, and C. Zhu, 2019: Roles of 681

tropical SST patterns during two types of ENSO in modulating wintertime 682

rainfall over southern China. Climate Dynamics, 52, 523-538. 683

Ying, J., P. Huang, and R. Huang, 2016: Evaluating the formation mechanisms of the 684

equatorial Pacific SST warming pattern in CMIP5 models. Advances in 685

Atmospheric Sciences, 33, 433-441. 686

Yuan, Y., and S. Yang, 2012: Impacts of Different Types of El Niño on the East Asian 687

Climate: Focus on ENSO Cycles. Journal of Climate, 25, 7702-7722. 688

Zhang, W., H. Li, F.-F. Jin, M. F. Stuecker, A. G. Turner, and N. P. Klingaman, 2015: 689

The Annual-Cycle Modulation of Meridional Asymmetry in ENSO’s 690

Atmospheric Response and Its Dependence on ENSO Zonal Structure. Journal 691

of Climate, 28, 5795-5812. 692

Zhang, X., and M. J. McPhaden, 2008: Eastern Equatorial Pacific Forcing of ENSO 693

Sea Surface Temperature Anomalies*. Journal of Climate, 21, 6070-6079. 694

695

696

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697

Figure 1. The two El Niño clusters identified by the FCM and the associated 698

DOMs: (a) the extreme El Niño cluster, which involves three historical extreme 699

El Niño events; (b) the moderate extreme El Niño cluster, which includes nine 700

historical moderate El Niño events; (c) the DOM for extreme El Niño (red curve), 701

moderate El Niño (blue curve), and neither (black curve). Stippling in (a, b) 702

indicates that the compositions are significant at the 95% confidence level, based 703

on the Student’s t-test. 704

705

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706

Figure 2. Spatial patterns of (a) SSTAs and (b) netQ during the developing phase 707

(May–December of the developing year) for extreme El Niños. Contours in (b) 708

are the SSTA tendencies during the developing phase (units: ℃ mon−1, with an 709

interval of 0.025 ℃ mon−1; zero contour thickened and negative dashed). (c–d) As 710

in (a–b) but for moderate El Niños. Stippling indicates that the compositions of 711

shaded values are significant at the 95% confidence level, based on the Student’s 712

t-test. (e), zonal distributions of equatorial (2.5°S–2.5N) netQ (blue curves) and 713

SSTA (red curves) for extreme (solid curves) and moderate (dashed curves) El 714

Niños. 715

716

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717

Figure 3. As in Figs. 2b and d but for netQ data from (a, c) GODAS and (b, d) 718

NCEP–NCAR. 719

720

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721

Figure 4. Scatter plot of difference of SSTAs versus that of netQ between eastern 722

Pacific (2.5°S–2.5N, 150°–90°W) and central Pacific (2.5°S–2.5N, 180°–150°W) 723

for each individual El Niño event during the developing phase. The horizontal 724

(vertical) red bar and the square box in the red bar denote the standard deviations 725

and mean of SSTAs (netQ ) only for moderate El Niños, respectively. The standard 726

deviations of SSTAs and netQ for moderate El Niños are indicated by red 727

horizontal and vertical bar, respectively. The red square box in the horizontal 728

(vertical) red bar denotes the mean of SSTAs (netQ ) for moderate El Niños. 729

730

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731

Figure 5. Hovmöller diagram for equatorial (2.5°S–2.5°N) (a, c) SSTAs and (b, d) 732

surface net heat flux anomalies during the developing year in (a, b) extreme and 733

(c, d) moderate El Niños. Contours in (a, c) denote the tendency of SSTAs (units: ℃ 734

mon−1, with an interval of 0.05 ℃ mon−1; zero contour thickened and negative 735

dashed), and in (b, d) denote the SSTAs (units: ℃, with an interval of 0.25℃; zero 736

contour thickened and negative dashed). Stippling indicates that the compositions 737

of shaded values are significant at the 95% confidence level, based on the 738

Student’s t-test. 739

740

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741

Figure 6. The ocean mixed-layer heat budget during the developing phase of (a) 742

extreme and (b) moderate El Niños based on GODAS. The red, blue and black 743

bars denote the regional-mean values in the eastern equatorial Pacific (EEP, 744

2.5°S–2.5N, 140°–90°W), the central equatorial Pacific (CEP, 2.5°S–2.5N, 745

180°–140°W), and their differences (EEP minus CEP). The O /C T t uQ , vQ , 746

wQ , netQ and resQ represent the tendency of mixed-layer temperature 747

anomalies, the mixed-layer zonal, meridional and vertical heat transport 748

anomalies, surface net heat flux anomalies, and residual term, respectively. Note 749

that the values on the y-axis are different between (a) and (b). 750

751

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37

752

Figure 7. Spatial patterns of (a) surface net shortwave radiation anomalies, (b) 753

surface latent heat flux anomalies, and (c) the sum of the two in extreme El Niños. 754

The black contours in (a, c) are the spatial patterns of precipitation anomalies 755

(units: ℃, with an interval of 0.5 mm day−1; zero contour thickened and negative 756

dashed) and surface net heat flux anomalies (units: W m−2, with an interval of 7.5 W 757

m−2; zero contour thickened and negative dashed), respectively. (d–f) As in (a–c), but 758

for moderate El Niños. Stippling indicates that the compositions of shaded values are 759

significant at the 95% confidence level, based on the Student’s t-test. 760

761

762

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38

763

Figure 8. Spatial patterns of the (a) reconstructed surface latent heat flux 764

anomalies based on Eq. (6) and (b–e) each factor involved in the surface latent heat 765

flux anomalies in extreme El Niños based on Eqs. (7)–(10) [(b) the Newtonian 766

cooling effect, and the atmospheric forcing effect due to anomalies in (c) surface wind 767

speed, (d) relative humidity and (e) surface stability]. Contours in (a–e) are the spatial 768

patterns of the original surface latent heat flux anomalies (units: W m−2, with an 769

interval of 7.5 W m−2; zero contour thickened and negative dashed), the SSTAs 770

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39

(units: ℃, with an interval of 0.2℃; zero contour thickened and negative dashed), the 771

surface wind speed anomalies (units: m s−1, with an interval of 0.15 m s−1; zero 772

contour thickened and negative dashed), the relative humidity anomalies (with an 773

interval of 7.5 × 10−3; zero contour thickened and negative dashed), and the surface 774

stability anomalies (units: ℃, with an interval of 0.15℃; zero contour thickened and 775

negative dashed), respectively. (f–j) As in (a–e) but for moderate El Niños. Stippling 776

indicates that the compositions of shaded values are significant at the 95% confidence 777

level, based on the Student’s t-test. 778

779

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40

780

Figure 9. Spatial patterns of the atmospheric forcing effect due to anomalies in (a) 781

surface zonal wind speed and (b) meridional wind speed in extreme El Niños. 782

Contours in (a, b) are the surface zonal wind anomalies and meridional wind 783

anomalies (units: m s−1, with an interval of 0.4 m s−1; zero contour thickened and 784

negative dashed), respectively. Vectors in (a, b) are the surface wind vector 785

anomalies (units: m s−1). (c, d) As in (a, b) but for moderate El Niños. Note that 786

the interval of contours in (c, d) is 0.2 m s−1, which is different from that in (a, b). 787

Stippling indicates that the compositions of shaded values are significant at the 95% 788

confidence level, based on the Student’s t-test. 789

790

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41

791

Figure 10. Spatial patterns of (a) relative humidity–SST feedback index (RSFI) and 792

(b) boundary-layer height–SST feedback index (BHFI). (c), vertical distribution 793

of equatorial (2.5°S–2.5N) RSFI in the eastern Pacific. Contours in (c) denote the 794

climatological relative humidity. Stippling indicates that the regressions are 795

significant at the 95% confidence level, based on the Student’s t-test. 796

797

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798

Figure 11. The major heat flux anomalies during the developing phase of (a) 799

extreme and (b) moderate El Niños. The red, blue and black bars denote the 800

regional-mean values in the eastern equatorial Pacific (2.5°S–2.5N, 140°–90°W), 801

the central equatorial Pacific (2.5°S–2.5N, 180°–140°W), and their differences 802

(eastern Pacific minus central Pacific). The netQ , SWQ , EQ , EOQ , EWQ , ERHQ , 803

and E TQ denote the surface net heat flux anomalies, the surface net shortwave 804

radiation anomalies, the surface latent heat flux anomalies, the Newtonian cooling 805

effect, and the atmospheric adjustments due to anomalies in surface wind speed, 806

relative humidity and surface stability, respectively. Note that the values on the 807

y-axis are different between (a) and (b). 808

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