W. Zhang , G. A. Vecchi , H. Murakami , G. Villarini L. Jia
Transcript of W. Zhang , G. A. Vecchi , H. Murakami , G. Villarini L. Jia
The Pacific Meridional Mode and the Occurrence of Tropical 1 Cyclones in the Western North Pacific 2
3 4
W. Zhang 1,2,*, G. A. Vecchi1,2, H. Murakami1,2, G. Villarini3, 5
L. Jia1,2 6
7 1National Oceanic and Atmospheric Administration/Geophysical Fluid 8
Dynamics Laboratory, Princeton, NJ, USA 9 2Atmospheric and Oceanic Sciences Program, Princeton University, 10
Princeton, NJ, USA 11 3 IIHR-Hydroscience & Engineering, The University of Iowa, Iowa City, 12
Iowa 13 14 15 16 17 18
*Corresponding author: 19 Wei Zhang 20 21 National Oceanic and Atmospheric Administration/Geophysical Fluid 22 Dynamics Laboratory, Princeton, NJ, USA, 08540 23 Phone: 609-452-5817 24 Email: [email protected] 25
26 27 28
29
1
Abstract 30
This study investigates the association between the Pacific Meridional Mode (PMM) 31
and tropical cyclone (TC) activity in the western North Pacific (WNP). It is found that 32
the positive PMM phase favors the occurrence of TCs in the WNP while the negative 33
PMM phase inhibits the occurrence of TCs there. Observed relationships are 34
consistent with those from a long-term preindustrial control experiment (1000 years) 35
of a high-resolution TC-resolving Geophysical Fluid Dynamics Laboratory (GFDL) 36
Forecast-oriented Low Ocean Resolution (FLOR) coupled climate model. The 37
diagnostic relationship between the PMM and TCs in observations and the model is 38
further supported by sensitivity experiments with FLOR. The modulation of TC 39
genesis by the PMM is primarily through the anomalous zonal vertical wind shear 40
(ZVWS) changes in the WNP, especially in the southeastern WNP. The anomalous 41
ZVWS can be attributed to the responses of the atmosphere to the anomalous 42
warming in the northwestern part of the PMM in the positive PMM phase, which 43
resembles a classic Matsuno-Gill pattern. Such influences on TC genesis are 44
strengthened by a cyclonic flow over the WNP. The significant relationship between 45
TCs and the PMM identified here may provide a useful reference for seasonal 46
forecasting of TCs and interpreting changes in TC activity in the WNP. 47
48
49
50
51 2
1. Introduction 52
Tropical cyclones (TC) are among the most destructive and costly natural disasters on 53
the earth (e.g., Rappaport 2000; Pielke Jr et al., 2008; Zhang et al., 2009). The 54
occurrence of TCs has long been the subject of scientific inquiry(e.g., Mitchell, 1932; 55
Gray, 1968; Henderson-Sellers et al., 1998; Simpson et al., 1998; Vitart and Stockdale, 56
2001; Liu and Chan, 2003; Klotzback, 2007; Chan, 2008; Sippel and Zhang, 2008; 57
Lin et al., 2014; Vecchi et al., 2014). Large-scale climate variations in various basins 58
affect the occurrence of TCs in the WNP by both local and remote forcing. In general, 59
variations in TC occurrence in the WNP are closely associated with the sea surface 60
temperature (SST) patterns such as the El Niño Southern Oscillation (ENSO) (Chan, 61
1985; Wu and Lau, 1992; Chan, 2000; Wang and Chan, 2002; Camargo and Sobel, 62
2005; Zhang et al., 2012), the Indian ocean warming (Du et al., 2010; Zhan et al., 63
2010; Zhan et al., 2014), the North Pacific Gyre Oscillation (Zhang et al., 2013) and 64
the Pacific Decadal Oscillation (PDO; Lee et al., 2012; Liu and Chan, 2012; 65
Girishkumar et al., 2014). Recently, it was suggested that the SST in the North 66
Atlantic also modulates TC activity in the WNP (Li et al., 2013; Huo et al., 2015). 67
The Pacific Meridional Mode (PMM) is here defined as the first Maximum 68
Covariance Analysis (MCA) Mode of SST and 10-m wind vectors in the Pacific, and 69
describes meridional variations in SST, winds and convection in the tropical Pacific 70
Ocean (Chiang and Vimont, 2004). The PMM bears marked resemblance to the 71
Atlantic Meridional Mode (AMM) in terms of its principal mechanisms, impacts and 72
3
interactions with extra-tropical climate systems (Chiang and Vimont, 2004). For 73
example, the North Pacific Oscillation (NPO) has been found to force the PMM, 74
while the North Atlantic Oscillation (NAO) acts to force the AMM (Vimont et al., 75
2003). 76
The PMM is closely associated with ENSO (Chang et al., 2007; Zhang et al., 2009; 77
Larson and Kirtman, 2013; Lin et al., 2014), with the PMM peaking around April and 78
May whereas ENSO usually reaches its peak in boreal winter (Chang et al., 2007; 79
Zhang et al., 2009; Larson and Kirtman, 2013; Lin et al., 2014). Previous studies have 80
indicated that the PMM may set the stage for the seasonal peak of ENSO (Larson and 81
Kirtman, 2014). However, the PMM can also exist independently of ENSO, with the 82
ENSO effect routinely removed through linear regression onto the cold tongue index 83
(CTI) when calculating the PMM index (Chiang and Vimont, 2004; Zhang et al., 2009; 84
Larson and Kirtman, 2014). 85
Previous research has found that the seasonal occurrence and accumulated energy of 86
hurricanes in the North Atlantic are strongly influenced by the AMM (Vimont and 87
Kossin, 2007; Smirnov and Vimont, 2010). More recently, Patricola et al., (2014) 88
examined the combined influence of the PMM and ENSO on hurricane activity in the 89
North Atlantic. Basically, the PMM consists of two parts: a northwestern part and a 90
southeastern part in the Eastern Pacific (Chiang and Vimont, 2004). During the 91
positive PMM phase, positive SST anomalies prevail in the northwestern part while 92
negative SST anomalies prevail in the southeastern part (Chiang and Vimont, 2004). 93
4
Such SST anomalies can be hypothesized to affect TC activity in the WNP by 94
modulating the large-scale circulation, much like the PMM has been found to 95
modulate weather and climate in East Asia (Li et al., 2010; Li and Ma, 2011). 96
Therefore, it is of great interest to examine whether the PMM modulates the 97
occurrence of TCs in the WNP. 98
The objectives of this study are thus: i) to assess whether and to what extent the PMM 99
modulates TC activity in the WNP, and ii) to dissect the mechanisms underpinning the 100
modulation based on both observations and model simulation. This study is expected 101
to enhance the understanding of TC activity in the WNP and to provide valuable 102
insights for seasonal forecasting of the occurrence of TCs over that region. Moreover, 103
since the PMM is linked to extra-tropical climate systems such as NPO (Rogers, 1981) 104
and NPGO (Di Lorenzo et al., 2010) which is the second principal mode of SST 105
anomalies in the North Pacific (Vimont et al., 2001), this study can play a role in 106
bridging the association of extra-tropical and tropical interactions. 107
The remainder of this paper is organized as follows. Section 2 presents the data and 108
methodology, while Section 3 discusses the results based on observations and 109
simulations. Section 4 includes the discussion and summarizes the main conclusions. 110
2. Data and Methodology 111 2.1 Data 112
The TC data are obtained from International Best Track Archive for Climate 113
Stewardship (IBTrACS; Knapp et al., 2010). The study period is 1961 - 2013 because 114
TCs after the 1960s are more reliable (Chan, 2008). The key meteorological variables 115
5
such as zonal and meridional wind fields, geopotential height, vorticity and relative 116
humidity are from the Japan Meteorology Agency (JMA) 55 reanalysis data (JRA-55). 117
To substantiate and reinforce the results, the National Centers for Environmental 118
Prediction and the National Center for Atmospheric Research (NCEP/NCAR; Kalnay 119
et al,. 1996) reanalysis data and the Modern Era Retrospective-analysis for Research 120
and Applications (MERRA) reanalysis are also employed. The JRA-55 is available 121
since 1958 on a global basis with a spatial resolution of 1.25° × 1.25°. It is based on a 122
new data assimilation system that reduces many of the problems reported in the first 123
JMA reanalysis (Ebita et al., 2011; Kobayashi et al., 2015). MERRA is produced by 124
the National Aeronautics and Space Administration (NASA) for the satellite era, using 125
a major new version of the Goddard Earth Observing System Data Assimilation 126
System Version 5 (GEOS-5) (Rienecker et al., 2011). MERRA data is only available 127
from 1979. The zonal vertical wind shear (|du/dz| or |uz|) is defined as the magnitude 128
of the differences in zonal wind between 200 hPa and 850 hPa level. The years used 129
in the above three reanalysis data are consistent with TC data. 130
Monthly estimates of SST are taken from the Met Office Hadley Centre 131
HadSST3.1.1.0 (Kennedy et al., 2011). The PMM index is calculated following the 132
method described in Chiang and Vimont (2004). In calculating it, the seasonal cycle 133
and the linear trend are first removed by applying a three-month running mean to the 134
data, and then subtracting the linear fit to the cold tongue index (CTI, Deser and 135
Wallace, 1987) from every single spatial point to remove correlations with El Niño 136
6
(Chiang and Vimont, 2004). The CTI is defined as the average SST anomaly over 137
6 °N - 6 °S, 180 - 90 °W minus the global mean SST (Deser and Wallace, 1987). 138
The peak season for TCs is defined as July-October. The results are consistent if we 139
slightly change the definition of the TC peak season from June to November or from 140
July to November (not shown). 141
2.2 Model 142
This study employs a newly developed high-resolution coupled climate model for 143
experiments, the Geophysical Fluid Dynamics Laboratory (GFDL) Forecast-oriented 144
Low Ocean Resolution Version of CM2.5 or FLOR (e.g., Vecchi et al., 2014; Jia et al., 145
2015;Yang et al., 2015). The aim in the development of FLOR was to represent 146
regional scales and extreme weather and climate events (e.g., TCs) keeping 147
computational costs relatively low. For these reasons, this model is characterized by 148
high-resolution land and atmosphere components but relatively low-resolution ocean 149
component (Vecchi et al., 2014). The atmosphere and land are the same as those of the 150
GFDL Climate Model version (CM) 2.5 (CM2.5; Delworth et al., 2012) with a spatial 151
resolution of 50 km × 50 km. The ocean and sea ice components of FLOR are similar 152
to those in the CM2.1 (Delworth et al., 2006) with a spatial resolution of 1×1 degree. 153
The relatively low spatial resolution of the ocean and sea ice components in FLOR 154
enables large ensembles and better efficiency for seasonal forecasting. This study 155
utilizes the flux-adjusted version of FLOR (FLOR-FA) for sensitivity experiments in 156
which climatological adjustments are applied to the model's momentum, enthalpy and 157
freshwater flux from the atmosphere to the ocean to give the model's SST and surface 158 7
wind stress a closer climatology to the observations over 1979 - 2012 (Vecchi et al., 159
2014). For more details about the FLOR model, please refer to Vecchi et al. (2014), 160
Jia et al. (2015) and references therein. 161
2.3 Control simulation 162
A 2500-year long control simulation was performed with the FLOR-FA by prescribing 163
radiative forcing and land use representative of 1860. These experiments are referred 164
to as "Pre-industrial" experiments with FLOR-FA. The control experiments are run for 165
a total of 2500 years, but here we focus on the first 1000 years for the analysis of 166
PMM and TCs for the sake of computing efficiency. The 500-year control simulation 167
by prescribing radiative forcing and land use representative of 1990 with FLOR-FA is 168
also analyzed on PMM-TC association. Because the PMM-TC association based on 169
FLOR-FA 1990 is consistent with that on FLOR-FA 1860, this study only shows 170
results based on FLOR-FA 1860. 171
2.4 Tracking algorithm 172
TCs in FLOR are tracked from 6-hourly model output by using the tracker developed 173
by Harris et al. (in prep) as implemented in Murakami et al. (2015, submitted to 174
Journal of Climate). The temperature anomaly averaged vertically over 300 and 500 175
hPa (ta) and sea level pressure (SLP) are key factors of this tracker. The tracking 176
procedures are as follows. 177
(1) Local minima of the smoothed SLP field are found. The location of the center is 178
properly adjusted by fitting a biquadratic to the SLP and locating the center at the 179
minimum. 180
8
(2) Closed contours is in an interval of 2 hPa (dp) around every single SLP low center. 181
The Nth contour is marked as the contiguous region surrounding a low central pressure 182
P with pressures lower than dp × N + P, as detected by a “flood fill” algorithm. It is 183
noted that the contours are not required to be circular and a maximum radius of 3,000 184
km is searched from each candidate low center. 185
(3) If the distances of contours are close enough, the low is counted as a TC center. In 186
this way, the tracker attempts to find all closed contours within a certain distance of 187
the low center and without entering contours belonging to another low. The maximum 188
10-m wind inside the set of closed contours is taken as the maximum wind speed at 189
that time for the storm. 190
(4) Warm cores are detected via similar processes: closed 1K contours for FLOR are 191
found surrounding the maximum ta within a TC's identified contours, no more than 1 192
degree from the low center. This contour must have a radius less than 3 degrees in 193
distance. If such a core is not found, it should not be marked as a warm-core low 194
center and the center is rejected. 195
(5) TC centers are combined into a track by taking a low center at time T – dt, 196
extrapolating its motion forward dt, and then seeking for storms within 750 km. It is 197
noted that a deeper low center has higher priority of tracking. 198
(6) The following criteria are required to pick up the final TCs. 199
a. A lifespan of at least 72 hours. 200
b. At least 48 cumulative (not necessarily consecutive) hours with a warm core. 201
9
c. At least 36 consecutive hours of a warm core with winds greater than 17.5 202
m s–1. 203
TC genesis is confined equatorward of 40 °N. TC density in the WNP is binned into 204
5° × 5° grid boxes at a 6-hour interval. 205
3. Results 206
The analysis results of the PMM-TC association are derived from observations, a 207
1000 year control experiment, and sensitivity experiments based on FLOR-FA. 208
3.1 Observations 209
The regressions of SST and 10-m wind fields onto the PMM index in observations are 210
shown in Figure 1a. There is a characteristic pattern to the PMM in the central and 211
eastern Pacific, with warming in the northwestern part (subtropical region) and 212
cooling in the southeastern part (tropical) (Figure 1a). The warming in the central 213
Pacific is in the vicinity of the western North Pacific and may affect TC activity there. 214
The regressions of TC track density onto the PMM index for 1961-2013 are largely 215
positive in the WNP in observations, indicating that TC activity is enhanced 216
(suppressed) in the WNP in the positive (negative) PMM phase (Figure 1b). In 217
addition, we calculate the correlation between the time series of the PMM index and 218
the TC frequency in the WNP for the period of 1961 - 2013. For each year, the PMM 219
index is calculated by averaging the monthly PMM index over the peak TC season 220
(July-October). The correlation coefficient between the two indices is 0.46, significant 221
at the 0.01 level (Figure 2). Although previous studies have argued that the occurrence 222
10
of the PMM is independent of ENSO (Zhang et al., 2009; Larson and Kirtman, 2014), 223
and the linear ENSO effect has been removed when calculating the PMM index, 224
partial correlation is calculated by controlling the Niño 3 index to further exclude the 225
linear influence of ENSO on the PMM-TC association. The partial correlation 226
coefficient is slightly more significant (0.48) after controlling for the ENSO effect 227
(not shown). 228
To analyze the observed relationship between WNP TC genesis and PMM, the WNP 229
is divided into five sub-regions following the definition of sub-regions in the WNP in 230
Wang et al. (2013): the South China Sea (SCS), northwestern part (NW), northeastern 231
part (NE), southwestern part (SW) and southeastern part (SE) (Figure 3). The SE part 232
has a relatively high density of TC genesis (Figure 3). The PMM index has a 233
significant positive correlation with TC frequency in the SE, NE and NW parts 234
(Figure 3). 235
To further assess which large-scale atmospheric conditions may be acting to modulate 236
the TC occurrence, a suite of variables associated with TC genesis (Chan, 2000; Wang 237
and Chan, 2002) based on JRA-55 are regressed onto the PMM index (Figure 4). 238
Chan and Liu (2004) found that the increase in local SST has no significant influence 239
on TC activity in the WNP. Indeed, the modulation of local large-scale circulation by 240
remote SST anomalies (e.g., ENSO) largely leads to changes in TC activity there 241
(Chan, 2000; Wang and Chan, 2002; Chan and Liu, 2004; Camargo and Sobel, 2005). 242
Therefore, instead of analyzing SST and maximum potential intensity, we analyze 243
11
600-hPa relative humidity, 850-hPa relative vorticity and zonal vertical wind shear 244
(ZVWS) for TC genesis. In general, the regressions of the PMM index on JRA-55, 245
NCEP/NCAR, and MERRA reanalysis data are consistent. Thus, we only show the 246
results from JRA-55 reanalysis data. The regression of ZVWS is characterized by 247
strong negative anomalies in a large portion of the WNP (0 - 20 °N, 120 °E - 180 °E), 248
which would act to enhance TC genesis (Figure 4). Further analysis indicates that the 249
changes in ZVWS arise from anomalous westerly (easterly) in 850 hPa (200 hPa) 250
level (Figure 4) although the anomalous westerly in 850 hPa is mainly located in the 251
western part of the WNP. Such anomalous winds in the lower and upper levels can 252
weaken the prevalent westerlies in the upper level (200 hPa) and the prevalent 253
easterlies (850 hPa) in the lower level over the WNP. We hypothesize that the large-254
scale circulation responses to the SST patterns of the PMM alter the Walker 255
Circulation, which is responsible for the changes in the lower and upper level wind 256
flow. The mechanisms underlying how the vertical wind shear is modulated by the 257
large-scale circulation are discussed in detail in Subsection 3.3. The anomalous 258
positive relative humidity in the SE part also supports higher TC genesis in the WNP 259
in MERRA. Although the MERRA reanalysis is only available from 1979, the 260
satellite-based data may be more reliable (not shown). The AMM pattern (the Atlantic 261
counterpart of PMM) also has a significant positive correlation with hurricane 262
frequency in the North Atlantic because of increased subtropical SST, convergence 263
12
and low sea level pressure and decreased vertical wind shear (Vimont and Kossin, 264
2007; Smirnov and Vimont, 2010). 265
266 3.2 Results from the long-term control run 267
The 1000-year control simulation of FLOR-FA with 1860 radiative forcing is 268
analyzed to further understand the PMM-TC association. The main purpose is to test 269
whether such PMM-TC association also holds for the long-term control simulation of 270
FLOR-FA, which would provide a dynamical framework in which to understand the 271
causes of this connection. The PMM index in the control experiment is also calculated 272
based on the method proposed in Chiang and Vimont (2004). The PMM in FLOR-FA 273
control simulation (Figure 5a) captures the fundamental features of the observed 274
PMM (Figure 1a), indicating that the FLOR-FA model is capable of simulating the 275
basic structure of the PMM in a fully-coupled numerical climate system. Despite 276
these encouraging comparison, the control experiment of FLOR-FA produces a 277
weaker cooling and 10-m wind fields in the southeastern part of PMM, and stronger 278
cooling northwest of the positive anomalies compared to observation. In addition, the 279
squared covariance fraction of the PMM in observation is 53% (Chiang and Vimont, 280
2004) whereas it is 30% in the control experiment, suggesting a weaker role of PMM 281
in the control experiment. 282
The regressions of TC track density on the PMM index are generally positive in the 283
WNP in control experiment (1000-year, Figure 5b), consistent with observations 284
(Figure 1b). However, the positive regressions are largely confined in the southeastern 285
13
WNP (Figure 5b). The correlation coefficient between the simulated PMM and WNP 286
TC frequency is 0.37 for the 1000-year simulation, significant at 0.01 level of 287
significance (Figure 6a). Figure 6b shows the histogram of the correlation coefficients 288
in moving 50-year chunks and all are positive. The correlation coefficient from the 289
observations is within the model spread. This suggests that the observed TC-PMM 290
association may be robust, as it is significant even in a long-term climate control 291
simulation. 292
The model shows negative anomalies in ZVWS in the southeastern part (0 – 20 °N, 293
150 °E–180 °E) of the WNP (Figure 7), similar to those based on observations 294
(Figures 4). There are positive anomalies of ZVWS westward of 150°E in the control 295
experiment, suggesting unfavorable condition for TC genesis there. This is 296
responsible for different spatial patterns for TC genesis between observation and 297
control simulation (Figure 3). Observations show that TC genesis is promoted in 298
almost all the sub-regions in observations (Figure 3). In contrast, the control 299
simulation shows that TC genesis is enhanced in the southeastern part while 300
suppressed in the southwestern sub-region of the WNP (Figure 3). It is noted that we 301
have also analyzed the 500-year FLOR-FA control with 1990 radiative forcing and the 302
results derived from both control runs are consistent in terms of the PMM pattern and 303
TC-PMM association. A possible reason responsible for discrepancy in TC genesis 304
between the control experiment and observations is the pre-industrial radiative forcing 305
in the control experiment. 306
14
In summary, the 1000-year control experiment produces quantitatively consistent 307
results with observation, with positive phases of the PMM conducive to WNP TC 308
genesis, and anomalous reductions of ZVWS during the positive PMM phases. 309
However, TC genesis exhibits different regional relationships between observations 310
and the control experiment, which may be explained by different anomalous ZVWS 311
patterns in model and observations. Interestingly, the regressions of relative humidity 312
in this control experiment is consistent with those in MERRA reanalysis (figure not 313
shown) in which positive anomalies are observed eastward of 140°E. In order to 314
further investigate the mechanisms underpinning how PMM modulates TC genesis in 315
the WNP, a set of sensitivity experiments have been performed using FLOR-FA and 316
will be discussed in next subsection. 317
3.3 Results from sensitivity experiments 318
To isolate the role of the PMM, a set of perturbation experiments were performed 319
with FLOR-FA using 1860 radiative forcing. In the first experiment, SST is restored 320
to a repeating annual cycle in the PMM region with a 5-day restoring timescale, 321
which is taken as the control run (CTRL) (Figure 8). The second experiment is set up 322
by prescribing the sum of the annual cycle of SST and the temporally constant SST 323
anomalies associated with positive PMM patterns (denoted as PPMM) in the PMM 324
region (Figure 8). After an initial 100-year spinup, both experiments are integrated for 325
100 years. The mask of the restoring SST is shown in Figure 8, with the coefficient 326
varying from 1 to 0 when moving from the center to the boundary of the masking 327
15
region. By subtracting the CTRL experiment from the PPMM experiment, one can 328
assess the net influence of the positive PMM phase on the climate system. 329
The WNP mean TC frequency during the peak TC season (JASO, July to October) in 330
the 100-year PPMM experiment (19.4) is significantly higher than the control 331
experiment (17.5) at 0.01 significance level (Table 1). The difference in WNP TC 332
frequency between the PPMM experiment (26.7) and CTRL (24.7) is also significant 333
for June-November (JJASON) (Table 1). To better represent the differences between 334
the two experiments, TC density is computed by binning TC centers onto each 5°×5° 335
grid box in the WNP. Positive anomalies of TC density are observed in the eastern 336
part of the WNP (Figure 9). However, the positive anomalies have higher magnitude 337
than the negative ones. These positive anomalies arise from an enhanced TC genesis 338
in the PPMM experiment (Figure 10). The occurrence of TC genesis in the PPMM 339
experiment is higher than that in the control run in the eastern part of the WNP 340
(Figure 10). These experiments corroborate that the positive PMM phases promote 341
TC genesis in the WNP, especially in the eastern portion of the WNP. A number of 342
studies have proposed mechanisms on how remote SST patterns affect TC genesis in 343
the WNP, including the Matsuno-Gill pattern (Matsuno, 1966; Gill, 1980), Pacific-344
East Asia teleconnections (Wang et al., 2000; Wang and Chan, 2002), the Philippine 345
anticyclone induced by Indian ocean warming (Xie et al., 2009; Ha et al., 2014) and 346
SST gradients (Zhan et al., 2013; Li and Zhou, 2014). These studies have emphasized 347
16
the importance of the Philippines anticyclone and monsoon trough in modulating TC 348
genesis and how SST anomalies modulate the large-scale circulation in remote areas. 349
To explain why TC genesis in the PPMM experiment is higher in the eastern part of 350
the WNP, the large-scale atmospheric factors related to TC genesis are analyzed. The 351
differences between the PPMM and control run resemble the regression of those 352
variables onto the PMM index in both control experiment and observations (Figure 353
11). This suggests that the SST pattern in the positive PMM phase and within that 354
particular box drives the modeled and observed TC genesis in the WNP, especially in 355
its eastern part. Specifically, negative anomalies of ZVWS are induced by the PPMM, 356
arising from westerly anomalies at the850 hPa level and easterly anomalies at the 200 357
hPa (Figure 11). These changes can be described as a change in the Walker 358
Circulation. The question is then related to the mechanisms that lead to the changes in 359
the Walker Circulation. It is known that the positive PMM pattern features a warming 360
in the northwestern part and a cooling in the southeastern part in the tropical eastern 361
Pacific (Figures 1, 5, 12). A cyclonic 850 hPa flow is forced by the anomalous 362
warming in the tropical central Pacific through the Matsuno-Gill response (Matsuno, 363
1966; Gill, 1980). The responses to anomalous positive PMM warming are quite 364
similar to the Matsuno-Gill pattern under asymmetric heating (Gill, 1980), showing 365
that a cyclonic pattern is located northwestward of the heating (Figure 12a). In 366
addition, the diabatic heating center can also be identified by negative outgoing 367
longwave radiation (OLR) anomalies (Figure 12a). The anomalous cyclonic flow 368
17
pattern in the WNP is more likely to cause a weaker Philippine anticyclone, a weaker 369
subtropical high and elongated monsoon trough, which are favorable conditions for 370
TC genesis in the WNP (Wang et al., 2000; Wang and Chan, 2002). Intensified low-371
level westerly and easterly flows move towards the PPMM heating center from east 372
and west, respectively (Figure. 12a). Such patterns are also pronounced in the profile 373
of zonal and vertical winds (Figure 12b). An updraft of the Walker circulation shifts to 374
the eastern part of the WNP (around 180°). Notice that the zonal wind is averaged 375
over 0° to 20°N when calculating vertical profile for the zonal and vertical wind 376
(Figure 12b). Anomalous easterlies (westerlies) in upper (lower) levels is elongated 377
from 140°E to 180°E (Figure 12b). Such tropospheric flow patterns weaken the 378
westerlies in the upper levels (e.g., 200 hPa) and easterlies in the lower levels (e.g., 379
850 hPa). The combined effect of changes in the lower and upper level winds is 380
responsible for the weakened zonal vertical wind shear in the eastern part of the WNP 381
(Figure 11), which leads to increased TC genesis there. Therefore, enhanced TC 382
genesis in the WNP can be attributed to weaker ZVWS, which may arise from the 383
responses of the atmosphere to the anomalous warming which is part of the positive 384
PMM pattern by the Matsuno-Gill mechanisms. 385
386 4. Discussion and conclusion 387
The Pacific Meridional Mode (PMM) has been the subject of heightened interest by 388
the scientific community because of its role in bridging across the extra-tropical and 389
tropical climate systems. It is thus of high scientific relevance whether the PMM is 390
18
linked to TCs in the WNP given that previous studies claimed that its counterpart 391
AMM is intimately associated with hurricane activity in the North Atlantic (Vimont 392
and Kossin, 2007; Smirnov and Vimont, 2010; Patricola et al., 2014). 393
This study has analyzed the observed and modeled association between the PMM and 394
TC activity in the WNP. Our results show that the positive PMM phase promotes the 395
occurrence of TCs in the WNP. There is a general consistency in the diagnostic TC-396
PMM relationship in observations and in a long-term control experiment (1000 years) 397
of FLOR-FA. Sensitivity experiments using the model show causality in the PMM/TC 398
relation. The modulation TC genesis by the PMM originates mainly from the 399
abnormal ZVWS in the WNP, especially in its southeastern portion as shown in the 400
control experiment and sensitivity experiments. The anomalous ZVWS can be 401
attributed to the responses to the atmosphere to the anomalous warming in the 402
positive PMM pattern through Matsuno-Gill mechanisms. Such results are supported 403
by the cyclonic flow in the Philippine Sea and relevant flow patterns over the Pacific 404
in the sensitivity experiments. 405
The PMM is linked to the climate modes in the North Pacific such as NPO and NPGO 406
(Chiang and Vimont, 2004). For example, NPO, which is the atmospheric component 407
of NPGO, tends to force the PMM (Chiang and Vimont, 2004). Therefore, PMM 408
bridges the extra-tropical and tropical climate systems. As shown in Zhang et al. 409
(2013), NPGO/NPO modulates the occurrence of TCs in the WNP and it plays an 410
even stronger role than ENSO and PDO based on observations. In addition, Chen et al. 411
19
(2015) reported that the Spring NPO can modulate TC activity in the WNP in the 412
following peak TC season. However, detailed mechanisms are yet to be unraveled. 413
This study may provide some hints to explain the impacts of NPGO or NPO on TCs 414
in the WNP. It is known that the PMM pattern is obtained by removing the effect of 415
ENSO via linearly removing of the cold tongue index (Deser and Wallace, 1990). TCs 416
in the WNP are affected by various climate modes such as ENSO, the Indian ocean 417
warming, NPGO, PDO, and the SST in the North Atlantic Ocean. This study has also 418
found that the PMM significantly modulates the occurrence of TCs in the WNP. An 419
on-going comprehensive study involving all of these SST patterns is analyzing their 420
relative roles in influencing TC genesis in the WNP. Given the important role of the 421
PMM in modulating the climate, the linkage between PMM and TC activity in other 422
ocean basins will be analyzed in our future study. Moreover, the results of this work 423
indicate that the predictability of the PMM is potentially of great value for the 424
prediction of TC activity; future studies will examine the predictability of the PMM 425
and TCs, by leveraging seasonal forecasting experiments with FLOR-FA. 426
427
Acknowledgments 428
The authors thank Xiaosong Yang and Andrew Wittenberg for their valuable 429
comments on an earlier version of this paper. WZ benefits from discussion with 430
Lakshmi Krishnamurthy on this study. The authors thank Seth Underwood and 431
Fanrong Zeng for their helpful assistance in experiments. 432
20
433
21
Reference 434 Camargo, S. J. and A. H. Sobel, 2005: Western North Pacific tropical cyclone 435
intensity and ENSO. Journal of Climate, 18, 2996-3006. 436 Chan, J. C. L., 1985: Tropical Cyclone Activity in the Northwest Pacific in Relation to 437
the El Niño Southern Oscillation Phenomenon. Monthly Weather Review, 113, 438 599-606. 439
Chan, J. C. L., 2000: Tropical cyclone activity over the western North Pacific 440 associated with El Niño and La Nina events. Journal of Climate, 13, 2960-2972. 441
Chan, J. C. L. and K. S. Liu, 2004: Global Warming and Western North Pacific 442 Typhoon Activity from an Observational Perspective. Journal of Climate, 17, 443 4590-4602. 444
——, 2008: A Simple Seasonal Forecast Update of Tropical Cyclone Activity. 445 Weather and Forecasting, 23, 1016-1021. 446
Chan, J.C.L., 2008: Decadal variations of intense typhoon occurrence in the western 447 North Pacific. Proceedings of the Royal Society A: Mathematical, Physical and 448 Engineering Science, 464, 249-272. 449
Chang, P., L. Zhang, R. Saravanan, D. J. Vimont, J. C. H. Chiang, L. Ji, H. Seidel, and 450 M. K. Tippett, 2007: Pacific meridional mode and El Niño—Southern Oscillation. 451 Geophysical Research Letters, 34, L16608. 452
Chen, D., Wang, H., Liu, J. and Li, G. , 2015: Why the spring North Pacific 453 Oscillation is a predictor of typhoon activity over the Western North Pacific. Int. J. 454 Climatol, in press. 455
Chiang, J. C. H. and D. J. Vimont, 2004: Analogous Pacific and Atlantic Meridional 456 Modes of Tropical Atmosphere–Ocean Variability. Journal of Climate, 17, 4143-457 4158. 458
Delworth, T. L., A. Rosati, W. Anderson, A. J. Adcroft, V. Balaji, R. Benson, K. Dixon, 459 S. M. Griffies, H.-C. Lee, R. C. Pacanowski, G. A. Vecchi, A. T. Wittenberg, F. 460 Zeng, and R. Zhang, 2012: Simulated Climate and Climate Change in the GFDL 461 CM2.5 High-Resolution Coupled Climate Model. Journal of Climate, 25, 2755-462 2781. 463
Delworth, T. L., A. J. Broccoli, A. Rosati, R. J. Stouffer, V. Balaji, J. A. Beesley, W. F. 464 Cooke, K. W. Dixon, J. Dunne, K. A. Dunne, J. W. Durachta, K. L. Findell, P. 465 Ginoux, A. Gnanadesikan, C. T. Gordon, S. M. Griffies, R. Gudgel, M. J. Harrison, 466 I. M. Held, R. S. Hemler, L. W. Horowitz, S. A. Klein, T. R. Knutson, P. J. 467 Kushner, A. R. Langenhorst, H.-C. Lee, S.-J. Lin, J. Lu, S. L. Malyshev, P. C. D. 468 Milly, V. Ramaswamy, J. Russell, M. D. Schwarzkopf, E. Shevliakova, J. J. Sirutis, 469 M. J. Spelman, W. F. Stern, M. Winton, A. T. Wittenberg, B. Wyman, F. Zeng, and 470 R. Zhang, 2006: GFDL’s CM2 Global Coupled Climate Models. Part I: 471 Formulation and Simulation Characteristics. Journal of Climate, 19, 643-674. 472
Deser, C. and J. M. Wallace, 1987: El Niño events and their relation to the Southern 473 Oscillation: 1925–1986. Journal of Geophysical Research: Oceans, 92, 14189-474 14196. 475
22
Deser, C. and J. M. Wallace, 1990: Large-Scale Atmospheric Circulation Features of 476 Warm and Cold Episodes in the Tropical Pacific. Journal of Climate, 3, 1254-477 1281. 478
Di Lorenzo, E., K. Cobb, J. Furtado, N. Schneider, B. Anderson, A. Bracco, M. 479 Alexander, and D. Vimont, 2010: Central Pacific El Nino and decadal climate 480 change in the North Pacific Ocean. Nature Geoscience, 3, 762-765. 481
Du, Y., L. Yang, and S.-P. Xie, 2010: Tropical Indian Ocean Influence on Northwest 482 Pacific Tropical Cyclones in Summer following Strong El Niño. Journal of 483 Climate, 24, 315-322. 484
Ebita, A., S. Kobayashi, Y. Ota, M. Moriya, R. Kumabe, K. Onogi, Y. Harada, S. 485 Yasui, K. Miyaoka, K. Takahashi, H. Kamahori, C. Kobayashi, H. Endo, M. Soma, 486 Y. Oikawa, and T. Ishimizu, 2011: The Japanese 55-year Reanalysis "JRA-55": an 487 interim report, SOLA, 7, 149-152. 488
Gill, A. E., 1980: Some simple solutions for heat-induced tropical circulation. 489 Quarterly Journal of the Royal Meteorological Society, 106, 447-462. 490
Girishkumar, M. S., V. P. Thanga Prakash, and M. Ravichandran, 2014: Influence of 491 Pacific Decadal Oscillation on the relationship between ENSO and tropical 492 cyclone activity in the Bay of Bengal during October–December. Climate 493 Dynamics, 1-11. 494
Gray, W. M., 1968: Global view of the origin of tropical disturbances and storms. 495 Monthly Weather Review, 96, 669-700. 496
Ha, Y., Z. Zhong, X. Yang, and Y. Sun, 2014: Contribution of East Indian Ocean 497 SSTA to Western North Pacific tropical cyclone activity under El Niño/La Niña 498 conditions. International Journal of Climatology,35,506-519. 499
Henderson-Sellers, A., H. Zhang, G. Berz, K. Emanuel, W. Gray, C. Landsea, G. 500 Holland, J. Lighthill, S. L. Shieh, P. Webster, and K. McGuffie, 1998: Tropical 501 cyclones and global climate change: A post-IPCC assessment. Bulletin of the 502 American Meteorological Society, 79, 19-38. 503
Huo, L., P. Guo, S. N. Hameed, and D. Jin, 2015: The role of tropical Atlantic SST 504 anomalies in modulating western North Pacific tropical cyclone genesis. 505 Geophysical Research Letters, 2015GL063184. 506
Jia, L., X. Yang, G. A. Vecchi, R. G. Gudgel, T. L. Delworth, A. Rosati, W. F. Stern, A. 507 T. Wittenberg, L. Krishnamurthy, S. Zhang, R. Msadek, S. Kapnick, S. 508 Underwood, F. Zeng, W. G. Anderson, V. Balaji, and K. Dixon, 2014: Improved 509 Seasonal Prediction of Temperature and Precipitation over Land in a High-510 Resolution GFDL Climate Model. Journal of Climate, 28, 2044-2062. 511
Kalnay, E., and Coauthors, 1996: The NCEP/NCAR 40-Year Reanalysis Project. Bull. 512 Amer. Meteor. Soc., 77, 437–471. 513
Kennedy, J. J., N. A. Rayner, R. O. Smith, D. E. Parker, and M. Saunby, 2011: 514 Reassessing biases and other uncertainties in sea surface temperature observations 515 measured in situ since 1850: 2. Biases and homogenization. Journal of 516 Geophysical Research: Atmospheres, 116, D14104. 517
23
Klotzback, P. J., 2007: Recent developments in statistical prediction of seasonal 518 Atlantic basin tropical cyclone activity. Tellus Series a-Dynamic Meteorology and 519 Oceanography, 59, 511-518. 520
Knapp, K. R., M. C. Kruk, D. H. Levinson, H. J. Diamond, and C. J. Neumann, 2010: 521 The International Best Track Archive for Climate Stewardship (IBTrACS). 522 Bulletin of the American Meteorological Society, 91, 363-376. 523
Larson, S. and B. Kirtman, 2013: The Pacific Meridional Mode as a trigger for ENSO 524 in a high-resolution coupled model. Geophysical Research Letters, 40, 3189-3194. 525
Larson, S. M. and B. P. Kirtman, 2014: The Pacific Meridional Mode as an ENSO 526 Precursor and Predictor in the North American Multimodel Ensemble. Journal of 527 Climate, 27, 7018-7032. 528
Lee, H. S., T. Yamashita, and T. Mishima, 2012: Multi-decadal variations of ENSO, 529 the Pacific Decadal Oscillation and tropical cyclones in the western North Pacific. 530 Progress in Oceanography, 105, 67-80. 531
Li, C. and H. Ma, 2011: Coupled modes of rainfall over China and the pacific sea 532 surface temperature in boreal summertime. Advances in Atmospheric Sciences, 28, 533 1201-1214. 534
Li, C., L. Wu, and P. Chang, 2010: A Far-Reaching Footprint of the Tropical Pacific 535 Meridional Mode on the Summer Rainfall over the Yellow River Loop Valley. 536 Journal of Climate, 24, 2585-2598. 537
Li, R. C. Y. and W. Zhou, 2014: Interdecadal Change in South China Sea Tropical 538 Cyclone Frequency in Association with Zonal Sea Surface Temperature Gradient. 539 Journal of Climate, 27, 5468-5480. 540
Li, X., S. Yang, H. Wang, X. Jia, and A. Kumar, 2013: A dynamical-statistical forecast 541 model for the annual frequency of western Pacific tropical cyclones based on the 542 NCEP Climate Forecast System version 2. Journal of Geophysical Research: 543 Atmospheres, 118, 12,061-12,074. 544
Lin, C.-Y., J.-Y. Yu, and H.-H. Hsu, 2014: CMIP5 model simulations of the Pacific 545 meridional mode and its connection to the two types of ENSO. International 546 Journal of Climatology, in press. 547
Lin, I. I., I.-F. Pun, and C.-C. Lien, 2014: 'Category-6' Supertyphoon Haiyan in Global 548 Warming Hiatus: Contribution from Subsurface Ocean Warming. Geophysical 549 Research Letters, 2014GL061281. 550
Liu, K. S. and J. C. L. Chan, 2003: Climatological characteristics and seasonal 551 forecasting of tropical cyclones making landfall along the South China coast. 552 Monthly Weather Review, 131, 1650-1662. 553
Liu, K. S. and J. C. L. Chan, 2012: Inactive Period of Western North Pacific Tropical 554 Cyclone Activity in 1998–2011. Journal of Climate, 26, 2614-2630. 555
Matsuno, T., 1966: Quasi-geostrophic motions in the equatorial area. J. Meteor. Soc. 556 Japan, 44, 25-43. 557
Mitchell, C. L., 1932: West Indian Hurricanes and Other Tropical Cyclones of the 558 North Atlantic of the North Atlantic Ocean. Monthly Weather Review, 60, 253-253. 559
24
Patricola, C. M., R. Saravanan, and P. Chang, 2014: The Impact of the El Niño–560 Southern Oscillation and Atlantic Meridional Mode on Seasonal Atlantic Tropical 561 Cyclone Activity. Journal of Climate, 27, 5311-5328. 562
Pielke Jr, R., J. Gratz, C. Landsea, D. Collins, M. Saunders, and R. Musulin, 2008: 563 Normalized hurricane damage in the United States: 1900–2005. Natural Hazards 564 Review, 9, 29-42. 565
Rappaport, E. N., 2000: Loss of life in the United States associatedwith recent 566 Atlantic tropical cyclones. Bull. Amer. Meteor.Soc., 81, 2065–2073. 567
Rienecker, M. M., M. J. Suarez, R. Gelaro, R. Todling, J. Bacmeister, E. Liu, M. G. 568 Bosilovich, S. D. Schubert, L. Takacs, G.-K. Kim, S. Bloom, J. Chen, D. Collins, 569 A. Conaty, A. da Silva, W. Gu, J. Joiner, R. D. Koster, R. Lucchesi, A. Molod, T. 570 Owens, S. Pawson, P. Pegion, C. R. Redder, R. Reichle, F. R. Robertson, A. G. 571 Ruddick, M. Sienkiewicz, and J. Woollen, 2011: MERRA: NASA’s Modern-Era 572 Retrospective Analysis for Research and Applications. Journal of Climate, 24, 573 3624-3648. 574
Rogers, J. C., 1981: The north Pacific oscillation. International Journal of Climatology, 575 1, 39-57. 576
Simpson, J., J. B. Halverson, B. S. Ferrier, W. A. Petersen, R. H. Simpson, R. 577 Blakeslee, and S. L. Durden, 1998: On the role of “hot towers” in tropical cyclone 578 formation. Meteorology and Atmospheric Physics, 67, 15-35. 579
Sippel, J. A. and F. Zhang, 2008: A Probabilistic Analysis of the Dynamics and 580 Predictability of Tropical Cyclogenesis. Journal of the Atmospheric Sciences, 65, 581 3440-3459. 582
Smirnov, D. and D. J. Vimont, 2010: Variability of the Atlantic Meridional Mode 583 during the Atlantic Hurricane Season. Journal of Climate, 24, 1409-1424. 584
Kobayashi, S., Y. Ota, Y. Harada, A. Ebita, M. Moriya, H. Onoda, K. Onogi, H. 585 Kamahori, C. Kobayashi, H. Endo, K. Miyaoka, and K. Takahashi , 2015: The 586 JRA-55 Reanalysis: General Specifications and Basic Characteristics. J. Meteor. 587 Soc. Japan, 93, 5-48, doi:10.2151/jmsj.2015-001. 588
Vecchi, G. A., T. Delworth, R. Gudgel, S. Kapnick, A. Rosati, A. T. Wittenberg, F. 589 Zeng, W. Anderson, V. Balaji, K. Dixon, L. Jia, H. S. Kim, L. Krishnamurthy, R. 590 Msadek, W. F. Stern, S. D. Underwood, G. Villarini, X. Yang, and S. Zhang, 2014: 591 On the Seasonal Forecasting of Regional Tropical Cyclone Activity. Journal of 592 Climate, 27, 7994-8016. 593
Vimont, D. J. and J. P. Kossin, 2007: The Atlantic Meridional Mode and hurricane 594 activity. Geophysical Research Letters, 34, L07709. 595
Vimont, D. J., D. S. Battisti, and A. C. Hirst, 2001: Footprinting: A seasonal 596 connection between the tropics and mid-latitudes. Geophysical Research Letters, 597 28, 3923-3926. 598
Vimont, D. J., J. M. Wallace, and D. S. Battisti, 2003: The Seasonal Footprinting 599 Mechanism in the Pacific: Implications for ENSO*. Journal of Climate, 16, 2668-600 2675. 601
25
Vitart, F. and T. N. Stockdale, 2001: Seasonal forecasting of tropical storms using 602 coupled GCM integrations. Monthly Weather Review, 129, 2521-2537. 603
Wang, B. and J. C. L. Chan, 2002: How strong ENSO events affect tropical storm 604 activity over the Western North Pacific. Journal of Climate, 15, 1643-1658. 605
Wang, B., R. Wu, and X. Fu, 2000: Pacific-East Asian Teleconnection: How Does 606 ENSO Affect East Asian Climate? Journal of Climate, 13, 1517-1536. 607
Wang, C., C. Li, M. Mu, and W. Duan, 2013: Seasonal modulations of different 608 impacts of two types of ENSO events on tropical cyclone activity in the western 609 North Pacific. Climate Dynamics, 40, 2887-2902. 610
Wu, G. X. and N. C. Lau, 1992: A Gcm Simulation of the Relationship between 611 Tropical-Storm Formation and Enso. Monthly Weather Review, 120, 958-977. 612
Xie, S.-P., K. Hu, J. Hafner, H. Tokinaga, Y. Du, G. Huang, and T. Sampe, 2009: 613 Indian Ocean Capacitor Effect on Indo–Western Pacific Climate during the 614 Summer following El Niño. Journal of Climate, 22, 730-747. 615
Yang, X., G. A. Vecchi, R. G. Gudgel, T. L. Delworth, S. Zhang, A. Rosati, L. Jia, W. F. 616 Stern, A. T. Wittenberg, S. Kapnick, R. Msadek, S. Underwood, F. Zeng, W. 617 Anderson, V. Balaji, 2015: Seasonal predictability of extratropical storm tracks in 618 GFDL’s high-resolution climate prediction model, Journal of Climate, in press. 619
Zhan, R., Y. Wang, and X. Lei, 2010: Contributions of ENSO and East Indian Ocean 620 SSTA to the Interannual Variability of Northwest Pacific Tropical Cyclone 621 Frequency. Journal of Climate, 24, 509-521. 622
Zhan, R., Y. Wang, and M. Wen, 2013: The SST Gradient between the Southwestern 623 Pacific and the Western Pacific Warm Pool: A New Factor Controlling the 624 Northwestern Pacific Tropical Cyclone Genesis Frequency. Journal of Climate, 26, 625 2408-2415. 626
Zhan, R., Y. Wang, and L. Tao, 2014: Intensified Impact of East Indian Ocean SST 627 Anomaly on Tropical Cyclone Genesis Frequency over the Western North Pacific. 628 Journal of Climate, 27, 8724-8739. 629
Zhang, L., P. Chang, and L. Ji, 2009: Linking the Pacific Meridional Mode to ENSO: 630 Coupled Model Analysis. Journal of Climate, 22, 3488-3505. 631
Zhang, Q., Q. Liu, and L. Wu, 2009: Tropical Cyclone Damages in China 1983–2006. 632 Bulletin of the American Meteorological Society, 90, 489-495. 633
Zhang, W., Y. Leung, and J. Min, 2013: North Pacific Gyre Oscillation and the 634 occurrence of western North Pacific tropical cyclones. Geophysical Research 635 Letters, 2013GL057691. 636
Zhang, W., H. F. Graf, Y. Leung, and M. Herzog, 2012: Different El Niño Types and 637 Tropical Cyclone Landfall in East Asia. Journal of Climate, 25, 6510-6523. 638
639
26
List of Tables 640
Table 1. TC frequencies in JASO and JJASON for PPMM and control experiment 641
respectively. Boldface numbers represent the differences that are statistically 642
significant and * represents 0.01 level of significance. 643
644
645
646
647
648
649
650
651
652
653
654
655
656
657
658
659
27
660
List of Figures 661
Figure 1. The regressions of (a) SST (unit: °C) and 10 m wind fields (unit: ms-1) and 662
(b) tropical cyclone track density onto the standardized PMM index. The spatial 663
domain in (a) is consistent with that in Chiang and Vimont (2004). 664
Figure 2. (a) The standardized time series of the yearly PMM index and WNP TC 665
frequency for the period 1961-2013 and (b) scatterplot of PMM vs WNP TC 666
frequency (dot) and fitted line (black line). The yearly PMM index and WNP TC 667
frequency are calculated by averaging over July-October . 668
Figure 3. The five sub-regions of TC genesis in the WNP. Blue dots represent TC 669
genesis locations in the period of 1961 - 2013. The text "obs" denotes the correlation 670
between PMM and TC frequency in observations whereas "ctrl" denotes that in 671
control run. The numbers following "obs" or "ctrl" denote correlation coefficients in 672
each subregion. "WNP(obs)" represents the correlation coefficient between PMM and 673
TC frequency in the WNP in observations while "WNP(ctrl)" denotes that in control 674
run (1000 years). *,**, and *** represent the significance level 0.1, 0.05 and 0.01, 675
respectively. 676
Figure 4. The regressions of 600 hPa relative humidity, 850 hPa relative vorticity 677
(×10-6), zonal vertical wind shear (ms-1), u850 (ms-1) and u200 (ms-1) onto the 678
PMM index based on JRA-55 reanalysis. The thick red lines are used to divide the 679
five subregions in the WNP. 680
28
681
Figure 5. Regression of (a) SST anomalies (°C) and 10 m wind fields (ms-1) and (b) 682
TC density onto the standardized PMM index in a 1000-yr control simulation of the 683
FLOR-FA. 684
Figure 6. (a) The scatterplot of PMM vs WNP TC frequency (blue dots) and fitted 685
line (black) in the control experiment, and (b) the histogram of correlation between 686
WNP TC frequency and PMM for every 50 years (the correlation between WNP TC 687
frequency and PMM based on observations is shown in the thin red bar). 688
Figure 7. The regressions of 600 hPa relative humidity, 850 hPa vorticity (×10-6), 689
zonal vertical wind shear (ms-1), u850 (ms-1) and u200 (ms-1) onto the PMM index 690
in the control experiment of FLOR-FA. The thick red lines are used to divide the five 691
subregions in the WNP. 692
Figure 8. The mask for the PMM region and the SST anomalies (°C) in positive PMM 693
phase added to the seasonal cycle in the experiment. 694
Figure 9. TC track density in the PPMM experiment (top panel), control experiment 695
(CTRL; middle panel) and the difference PPMM - CTRL (bottom panel). 696
Figure 10. As in Fig.9, but for TC genesis. 697
Figure 11. The differences in 600 hPa relative humidity, 850 hPa relative vorticity 698
(×10-6), ZVWS (200 - 850 hPa, unit: ms-1), u850 (ms-1) and u200 (ms-1) between 699
PPMM and control experiments. The thick red lines are used to divide the five 700
subregions in the WNP. 701
29
Figure 12. (a) The differences in 850 hPa wind fields (vector, unit: ms-1) and OLR 702
(contour, unit: W·m-2) between PPMM and CTRL experiments with FLOR-FA, and 703
the SST pattern of the positive PMM pattern (shading, unit: °C) and (b) the vertical 704
profile of zonal wind (ms-1) from 1000 hPa to 100 hPa level (the zonal wind is 705
averaged over 0° and 20°N) between PPMM and CTRL experiments. The vertical 706
velocity is multiplied by -100 in (b). 707
708
709 710
30
Table 1. TC frequencies in JASO and JJASON for PPMM and control experiment 711 (CTRL) respectively. Boldface numbers represent the differences that are statistically 712 significant, with *** representing results significant at the 0.01 level based on t-test. 713 Frequency JJASON JASO PPMM 26.7 19.4 CTRL 24.7 17.5 PPMM - CTRL 2.0*** 1.9***
714
31
Figures 715
Figure 1. The regressions of (a) SST (unit: °C) and 10 m wind fields (unit: ms-1) and 716
(b) tropical cyclone track density onto the standardized PMM index. The spatial 717
domain in (a) is consistent with that in Chiang and Vimont (2004). 718
719
32
720
721 Figure 2. (a) The standardized time series of the yearly PMM index and WNP TC 722 frequency for the period 1961-2013 and (b) scatterplot of PMM vs WNP TC 723
33
frequency (dot) and fitted line (black line). The yearly PMM index and WNP TC 724 frequency are calculated by averaging over July-October . 725 726
34
727
Figure 3. The five sub-regions of TC genesis in the WNP. Blue dots represent TC 728
genesis locations in the period of 1961 - 2013. The text "obs" denotes the correlation 729
between PMM and TC frequency in observations whereas "ctrl" denotes that in 730
control run. The numbers following "obs" or "ctrl" denote correlation coefficients in 731
each subregion. "WNP(obs)" represents the correlation coefficient between PMM and 732
TC frequency in the WNP in observations while "WNP(ctrl)" denotes that in control 733
run (1000 years). *,**, and *** represent the significance level 0.1, 0.05 and 0.01, 734
respectively. 735
35
736
737 Figure 4. The regressions of 600 hPa relative humidity, 850 hPa relative vorticity 738 (×10-6), zonal vertical wind shear (ms-1), u850 (ms-1) and u200 (ms-1) onto the PMM 739 index based on JRA-55 reanalysis. The thick red lines are used to divide the five 740 subregions in the WNP. 741
36
742
743 Figure 5. Regression of (a) SST anomalies (°C) and 10 m wind fields (ms-1) and (b) 744 TC density onto the standardized PMM index in a 1000-yr control simulation of the 745 FLOR-FA. 746 747 748 749 750
37
751 Figure 6. (a) The scatterplot of PMM vs WNP TC frequency (blue dots) and fitted line 752 (black), and (b) the histogram of correlation between WNP TC frequency and PMM 753 for every 50 years (the correlation between WNP TC frequency and PMM based on 754 observations is shown in the thin red bar) in the control experiment of FLOR-FA. 755 756
38
757 Figure 7. The regressions of 600 hPa relative humidity, 850 hPa vorticity (×10-6), 758 zonal vertical wind shear (ms-1), u850 (ms-1) and u200 (ms-1) onto the PMM index in 759 the control experiment of FLOR-FA. The thick red lines are used to divide the five 760 subregions in the WNP. 761 762
39
763
Figure 8. The mask for the PMM region and the SST anomalies (°C) in positive PMM 764 phase added to the seasonal cycle in the experiment. 765 766 767 768
40
769 Figure 9. TC track density in the PPMM experiment (top panel), control experiment 770 (CTRL; middle panel) and the difference PPMM - CTRL (bottom panel). 771 772 773
41
774 Figure 10. As in Fig.9, but for TC genesis. 775
776
42
777 Figure 11. The differences in 600 hPa relative humidity, 850 hPa relative vorticity 778 (×10-6), ZVWS (200 - 850 hPa, unit: ms-1), u850 (ms-1) and u200 (ms-1) between 779 PPMM and control experiments. The thick red lines are used to divide the five 780 subregions in the WNP. 781 782
43
783 Figure 12. (a) The differences in 850 hPa wind fields (vector, unit: ms-1) and OLR 784 (contour, unit: W·m-2) between PPMM and CTRL experiments with FLOR-FA, and 785 the SST pattern of the positive PMM pattern (shading, unit: °C) and (b) the vertical 786 profile of zonal wind (ms-1) from 1000 hPa to 100 hPa level (the zonal wind is 787 averaged over 0° and 20°N) between PPMM and CTRL experiments. The vertical 788 velocity is multiplied by -100 in (b). 789 790 791
44