The variability of observed tropical cyclone (TC) activity (i.e., genesis, track, and landfall) in the western North Pacific (WNP) is examined in relation to the various categories of the Madden–Julian oscillation (MJO) during summer (June–September) for the period 1979–2004. The MJO categories are defined based on the empirical orthogonal function analysis of outgoing longwave radiation data.
The number of TCs increases when the MJO-related convection center is located in the WNP. The axis of a preferable genesis region systematically shifts like a seesaw in response to changes in the large-scale environments associated with both the eastward and northward propagation of the MJO and the intraseasonal variability of the WNP subtropical high. Furthermore, the authors show that the density of TC tracks in each MJO category depends on the systematic shift in the main genesis regions at first order. Also, the shift is affected by the prevailing large-scale steering flows in each MJO category. When the MJO-related convection center is found in the equatorial Indian Ocean (the tropical WNP), a dense area of tracks migrates eastward (westward). The effects of extreme ENSO events and the variations occurring during ENSO neutral years are also examined.
A statistical analysis of TC landfalls by MJO category is applied in seven selected subareas: the Philippines, Vietnam, South China, Taiwan, East China, Korea, and Japan. While a robust and significant modulation in the number of TC landfalls is observed in south China, Korea, and Japan, the modulation is marginal in the remaining four subareas.
Tropical atmospheric circulation shows signs of a significant spectral peak in the intraseasonal spectral band, indicating the importance of intraseasonal variability for tropical weather. The most dominant tropical intraseasonal oscillation is known as the Madden–Julian oscillation (MJO: Madden and Julian 1971). The MJO represents eastward-propagating quasiperiodic signals of circulation and convection. It originates over the Indian Ocean and moves eastward across the Maritime Continent to the Pacific Ocean. The propagating features are shown on a planetary scale with a broadband spectral peak ranging from 30 to 90 days. Extensive efforts have been made to understand the origin and dynamical/physical characteristics of the MJO and its impact on global and regional climate [for a review see Zhang (2005)]. The MJO interacts with the Asian–Australian monsoon (e.g., Lawrence and Webster 2002, and references therein), global tropical cyclone (TC) activity (e.g., Nakazawa 1986; Liebmann et al. 1994; Molinari et al. 1997; Molinari and Vollaro 2000; Maloney and Hartmann 2000a, b, 2001; Hall et al. 2001; Straub and Kiladis 2003; Bessafi and Wheeler 2006; Frank and Roundy 2006; Harr 2006; Ho et al. 2006), and cold surge occurrences and winter precipitation in East Asia (e.g., Jeong et al. 2005, 2008).
A possible linkage between the MJO and global TC activity was firstly detected by Gray (1979), even though other intraseasonal variability having different time scales, as well as the MJO, is involved in the linkage. He found that the period of active TC genesis over the globe tends to be clustered over a period of 2–3 weeks, followed by a comparable period of inactive TC genesis. Subsequently, a number of studies have been performed to clarify the relationship between the MJO and TCs in the global tropics. Over the western North Pacific (WNP), Nakazawa (1986) documented the clustering of TC occurrences according to the 30–60 day oscillation using outgoing longwave radiation (OLR) data obtained in 1979. Liebmann et al. (1994) extended this research using an additional data period and showed evidence for modulation of TC genesis by the MJO. They suggested that TC genesis tends to be frequent during the MJO convective period. However, the ratio of intense systems (i.e., tropical storms and typhoons) to weak systems (i.e., tropical depressions) seems to be nearly constant regardless of the convective and/or dry periods. Recently, Harr (2006) further identified the MJO years that exhibit the temporal clustering of TCs in the WNP and those that do not exhibit it, concluding that other factors that contribute to TC genesis override the inhibiting impacts due to the MJO during the latter years, while the temporal clustering is due to the significant decrease in TC occurrence during the suppressed convective period of the MJO during the former years.
To explain the enhanced TC genesis during the MJO convective period, some recent studies have investigated the genesis mechanism by means of low-level barotropic wave dynamics over monsoon confluence regions where the monsoon westerlies impinge on the trade easterlies (e.g., Sobel and Maloney 2000; Hartmann and Maloney 2001; Maloney and Hartmann 2001; Aiyyer and Molinari 2003; Maloney and Dickinson 2003). Also, this mechanism can be explained as a barotropic wave accumulation associated with variations of the low-level zonal wind. Sobel and Maloney (2000) examined the time-mean barotropic wave activity flux at 850 hPa and found that it increases when the MJO is in a westerly (i.e., convective) phase in the WNP. In an extended study, Maloney and Hartmann (2001) explained the modulation of TCs by the MJO in terms of low-level barotropic dynamics. When the MJO westerly anomalies at 850 hPa occur in the tropical WNP, the barotropic wave accumulation, from the mean flow to the eddy kinetic energy, becomes active. This process is associated with an enhanced surface convergence and 850-hPa cyclonic shear of the monsoon flow so that active eddy growth in such an environment creates favorable conditions for TC genesis. The converse is true during an anomalous MJO easterly phase. A study using a linear shallow-water model by Aiyyer and Molinari (2003) further confirmed that the off-equatorial disturbances, approximately 1000–2000 km in scale, develop in the presence of the MJO, which could serve as precursors to TCs. They said that this process may be particularly relevant to cyclogenesis in the tropical WNP.
In addition to the aforementioned studies that focused on the genesis or occurrence frequency of TCs, some studies have delineated the variability of TC tracks, for example, the geographical prevalence of TC occurrence over the East and Southeast Asia regions in relation to the tropical intraseasonal oscillation. Harr and Elsberry (1991, 1995) investigated the clustering of TC tracks in the WNP associated with variations of the monsoon circulation, having an intraseasonal time scale. They applied a fuzzy clustering method, which is a generalization of cluster analysis [refer to Harr and Elsberry (1995) for more detailed information], to classify distinct 700-hPa circulation patterns and then tried to link circulation patterns with TC track descriptive characteristics such as “straight moving,” “recurving,” and “inactive.” Recently, Delk (2004) briefly described TC tracks in the WNP in relation to the submonthly mode (i.e., a 15–25-day band of the intraseasonal oscillation). However, to the authors’ knowledge, there has been no comprehensive discussion of spatial variations of TC activity (i.e., genesis locations, tracks, and landfalls) in the WNP connected to the evolution of the MJO in the time range of 30–90 days. Thus, parts of this study aim to provide such an analysis.
East and Southeast Asian countries are hit by several TCs every year (cf. Kim et al. 2005a). Since TCs bring heavy rainfall and strong wind gusts that result in severe natural disasters, they invariably result in the loss of human life and property. Therefore, it is important to improve the accuracy of forecasts of the monthly or seasonal activity of TC landfalls. For these long-lead forecasts, it is essential to understand the activity of landfalling TCs associated with atmospheric/oceanic low-frequency variability at time scales ranging from subseasonal to interannual. While some research has been conducted to obtain statistics for landfalling TCs associated with the El Niño–Southern Oscillation (e.g., Saunders et al. 2000; Elsner and Liu 2003; Liu and Chan 2003; Wu et al. 2004; Fudeyasu et al. 2006) and the Antarctic Oscillation (e.g., Ho et al. 2005), no effort has been spared to explore the relationship between landfalling TCs and the MJO. Hence, parts of this study examine the statistics of landfalling TCs for each coastal area in every MJO category.
ENSO is known to be the most important planetary-scale phenomenon that affects interannual variations of TC activity in the WNP. The location of TC genesis shifts with the ENSO phase (e.g., Chia and Ropelewski 2002, and references therein) and track and landfall area do as well (e.g., Wang and Chan 2002; Wu and Wang 2004; Wu et al. 2004; Camargo and Sobel 2005; Camargo et al. 2007; Fudeyasu et al. 2006), showing that ENSO strongly modulates spatial variations of TC activity on an interannual time scale. Because this study aims mainly to investigate the spatial variations, the authors have tried to separate the impacts of the MJO from those related to ENSO phases.
This paper is organized into five sections as follows. Section 2 describes the datasets used, the methods of categorizing MJO evolution, and the placing of TCs into each MJO category. Section 3 discusses the main results that include the variability of TC genesis and tracks, explains the transitional characteristics from one category to the other and the statistics of TC landfalls, and gives an analysis of the effects of ENSO. Finally, a summary and discussion are presented in sections 4 and 5.
2. Data and analysis methods
Daily interpolated OLR obtained from the polar orbiting satellites of the National Oceanic and Atmospheric Administration (NOAA) has been utilized for identifying the structure and phase of the MJO (Liebmann and Smith 1996). The dataset is on a 2.5° × 2.5° latitude–longitude grid and is available for the period from June 1974 to the present, except for the period from 17 March to 31 December 1978. The daily horizontal winds at seven pressure levels (i.e., 850, 700, 600, 500, 400, 300, and 200 hPa), the relative vorticity at 850 hPa, and the geopotential heights at 500 hPa obtained from the National Centers for Environmental Prediction–National Center for Atmospheric Research (NCEP–NCAR) reanalysis have been analyzed to extract the large-scale circulation characteristics (Kalnay et al. 1996).
The Niño-3.4 (5°S–5°N, 120°–170°W) index has been chosen as an El Niño index, which is obtained from the NOAA monthly 2° × 2° extended reconstructed sea surface temperature (SST) anomalies, based on the 1971–2000 base period (Smith and Reynolds 2004).
The TC information used in this study has been obtained from the archive of the Regional Specialized Meteorological Centers–Tokyo Typhoon Center. This dataset contains a 6-hourly record (a 3-hourly record in some cases) of the latitude/longitude position of the low center, minimum central pressure value, and maximum 10-min-averaged surface wind speed (υmax), for all tropical storms (υmax ≥ 17 m s−1) and typhoons (υmax ≥ 33 m s−1) during the period 1951–2004. Therefore, the term TC covers both tropical storms and typhoons.
In the present study, the analysis period is confined to summer (June–September) from 1979 to 2004 because TC activity in the WNP is known to be strong during summer (Ho et al. 2004), and satellite-derived data have been routinely incorporated into the NCEP–NCAR assimilation system since 1979 (Kalnay et al. 1996).
b. Analysis methods
1) Determination of the MJO category
The space–time wave filter (Hayashi 1971; Wheeler and Kiladis 1999) has been applied to the OLR data over the circumglobal tropical domain (20°S–20°N) in order to extract the eastward-propagating signals of the MJO. The wavenumber of the filter ranges from 0 to 5 and the period ranges from 30 to 90 days. Within these ranges of wavenumber and period, a large spectral power of the eastward-propagating waves was observed (see Fig. 3 of Wheeler and Kiladis 1999). After the filtering is carried out, an empirical orthogonal function (EOF) analysis was performed on the MJO-filtered OLR only for summer, as in Matthews (2000).
Figure 1 shows the two leading EOFs (i.e., EOF1 and EOF2) and their associated principal component (PC) time series (i.e., PC1 and PC2). While EOF1 exhibits negative OLR anomalies (i.e., strong convection) in the tropical Indian Ocean and positive anomalies (i.e., weak convection) from the Indian subcontinent to the western Pacific (Fig. 1a), EOF2 exhibits strong convection from the Arabian Sea to the Maritime Continent and weak convection from the Indochina peninsula to the Philippine Sea (Fig. 1b). In general, these two EOFs illustrate a quadrature phase relationship in the spatial domain with a similar magnitude in their explained variance. In the temporal domain, PC1 leads PC2 by about 90° (Fig. 1c). It is evident that the two modes represent a propagating wave phenomenon (Zhang and Hendon 1997). Furthermore, it is noted that the propagating characteristic appears to be northward as well as eastward, although the space–time filtering used to extract the MJO mode is based on zonal propagation alone. This is meaningful because the northward propagation of the intraseasonal oscillation is strongest over the Indian Ocean and the WNP during summer (Wang and Rui 1990; Kemball-Cook and Wang 2001).
The phase and amplitude indices of the propagation vector can be expressed as tan−1[PC2(t)/PC1(t)] and PC12(t) + PC22(t), respectively. Here, four active categories—A, B, C, and D—of the MJO are defined according to the phase index with the constraint that the amplitude is greater than one standard deviation. Category A denotes the first quadrant of the PC1–PC2 plane where the phase index is located between 0° and 90°. The remaining three categories are denoted by the second (90°–180°), third (180°–270°), and fourth (270°–360°) quadrants of the PC1–PC2 plane. In addition, an inactive category—NONE—of the MJO is defined for the residual days.
The sensitivity of the amplitude threshold is examined by changing it from 0.5 to 1.5. Table 1 shows the number of MJO days in each category according to variations in the amplitude threshold. If the threshold is set up at 0.5 standard deviation, the percentage of active MJO days is nearly 90% of the whole period. This is a somewhat unacceptable condition because the MJO is present nearly all of the time during summer. Although the major conclusions are little affected by setting up this loose threshold, the greater possibility of contamination of the MJO signal by the other variables may be unavoidable. By contrast, the percentage of active MJO days is only 34.6% when the threshold is set up at 1.5 standard deviation. While this strict condition is more evidently representative of MJO-related variability, a period of scant MJO activity may restrict the limit of applicable time. On that account, a more “standard” threshold of one standard deviation, which includes 64% of the whole period, is adopted here (cf. Wheeler and Hendon 2004; Bessafi and Wheeler 2006). However, it should be mentioned that defining the active MJO period cannot help avoiding its inherent artificiality.
Figure 2 shows the four categories of the composite MJO life cycle represented by the OLR anomalies. The anomaly values used in the composite maps were obtained by subtracting the season mean value. Overall, the sequence of the four categories represents both eastward- and northward-propagating characteristics. In category A, anomalous deep convection dominates in the tropical Indian Ocean (Fig. 2a). As the convection center propagates both east and north, the WNP belongs to the convective phase in category C, showing an opposite structure compared to category A (Fig. 2c). Such examples of opposite OLR distributions are similarly found in the vast areas extending from the Arabian Sea to the Indochina peninsula in the case of categories B and D (Figs. 2b and 2d).
2) Comparison with the RMM index
Although the definition of the MJO in the present study is widely used in many studies (e.g., Wheeler and Kiladis 1999; Straub and Kiladis 2003; Bessafi and Wheeler 2006; Frank and Roundy 2006), some caveats must be given. There is another MJO index, called a real-time multivariate MJO (RMM) index, defined by Wheeler and Hendon (2004), that has been applied to monitoring and predicting MJO activity. The RMM index is also defined by two leading PCs (i.e., RMM1 and RMM2) of the EOF analysis technique as the MJO index (i.e., PC1 and PC2) used in this study except that it is extracted from the combined fields of daily (with long-time-scale components removed) zonal winds at 850 and 200 hPa and OLR averaged between 15°S and 15°N without applying the bandpass time filter. Power spectra of the RMM (see Fig. 2 of Wheeler and Hendon 2004) show a large spectral peak at 30–80 days, which is typically associated with the MJO. Thus, it is necessary to compare the MJO index used in this study with the RMM index to qualify the results of this study.
Figure 3 shows the PC1 and RMM1 during the whole analysis period. The two indices fluctuate analogously, having a correlation coefficient of 0.66. However, the two indices show a large discrepancy at some periods (usually during weak MJO periods), resulting in the ambiguity that a particular day belongs to completely different MJO categories. One reason why this study did not use the RMM is because it generates rather unstable phase propagation (i.e., retrograde phase transition) due to day-to-day noise in the time series, which is not presented in the MJO index used in this study. The presence of day-to-day noise may be due to the existence of high-frequency spectral powers less than 30 days. In this regard, the RMM index may not be suitable for this study, which mainly aims to clarify the impact of the MJO at the 30–90-day spectral band. Thus, the MJO index obtained from the EOF analysis of the space–time filtered OLR was utilized to isolate the effect of the MJO spectral band at 30–90 days.
3) Analyses of TC activity
To examine the MJO–TC relationship, TCs are put into each MJO category based on the date of their genesis. If the TCs occur in any two consecutive MJO categories after they propagate and develop, they belong to the first category, which is defined based on their genesis time. In addition, analyses are performed separately with respect to early summer (June–July, hereafter JJ) and late summer (August–September, hereafter AS) to consider the timing of the MJO categories.
The genesis locations and tracks of TCs, and the frequency of TC passage (TPF), are also examined. The TPF is the value obtained by dividing the number of TC occurrences in each 5° × 5° latitude–longitude grid by the total number of the TCs in each MJO category. In other words, the TPF denotes the probability density distribution of TCs in the spatial domain (see Ho et al. 2004).
To consider the effect of ENSO on TC activity, El Niño (La Niña) years were chosen when the summer-mean Niño-3.4 index was greater (less) than 0.5°C (−0.5°C). The selected years were 1982, 1987, 1991, 1994, 1997, 2002, and 2004 for El Niño and 1988, 1998, and 1999 for La Niña. The other 16 years were classified as neutral years.
Following Hall et al. (2001), a statistical test was performed to test whether the number of TC geneses and landfalls for each MJO category were significantly different from the uniformly distributed value in each category. If we assume that the probability of TC genesis or landfall on any particular day is constant, the probability distribution can be regarded as a binomial distribution. The test statistic is Z = (p̂ − p0)/p0(100 − p0)/N in which p0, p̂, and N are the expected and observed percentages of TC genesis and landfall days and the number of days for a particular MJO category, respectively. The test statistic Z generally follows a Gaussian normal distribution with an expected value 0 and variance 1 when the sampling day N is large enough.
Figure 4 presents the locations of TC genesis during summer (Figs. 4a–d), JJ (Figs. 4e–h), and AS (Figs. 4i–l) for each MJO category. The horizontal and vertical lines delineate four quadrants; these lines intersect at the mean position (15.9°N, 138.9°E) of all 413 TCs during summer, at 14.6°N, 136.5°E for all 151 TCs during JJ, and at 16.6°N, 140.2°E for all 262 TCs during AS. Numbers significantly above or below the climatology by statistics, as in Hall et al. (2001), are marked with asterisks or cross symbols, respectively.
The number of geneses increases from category A to C and decreases from category C to A during summer (48→65→81→72) and JJ (16→27→40→26). The numbers of geneses in categories A (C) are significantly fewer (more) over the 90% confidence level than the climatological average. These changes coincide with the variations of the composite OLR anomalies in the WNP (Fig. 2). These results are also consistent with previous studies (e.g., Nakazawa 1986; Liebmann et al. 1994). To check the seasonal difference of MJO-related variations in the total genesis number, it is shown separately for JJ and AS (Figs. 4e–l). The changes from category A to D are smaller during AS (32→38→41→46) than during JJ (16→27→40→26), though the number of geneses is large, indicating that the aforementioned variations in the number of geneses during summer can be mainly attributed to that during JJ. It is noted that the modulation of basinwide TC genesis by the MJO spectral band is rather weak during AS, suggesting that there are other large-scale contributing factors that are important to TC genesis. These include off-equatorial tropical depression (TD) type disturbances that have the characteristic time scales of synoptic waves (i.e., 3–10 days) (e.g., Lau and Lau (1990); Takayabu and Nitta (1993); Chang et al. (1996)), which may be initiated by the scale contraction of mixed Rossby–gravity (MRG) waves within a monsoon confluent region (e.g., Sobel and Bretherton 1999; Kuo et al. 2001; Dickinson and Molinari 2002; Aiyyer and Molinari 2003) or by Rossby wave energy dispersion in the wake of a preexisting TC (e.g., Briegel and Frank 1997; Ritchie and Holland 1999; Sobel and Bretherton 1999; Li et al. 2003; Li and Fu 2006), and the intraseasonal variability of the monsoon circulation and convection that have submonthly time scales (e.g., Hartmann et al. 1992; Fukutomi and Yasunari 1999; Delk 2004; Ko and Hsu 2006). Although these factors are not the main scope of this study, we suggest that consideration of these factors together with the MJO would be necessary for a better understanding of variations in TC genesis in further studies.
Spatial variations of the major locations of TC genesis on a subbasin scale are detected as clearly as the basinwide variations in the total number. The axis of preferable genesis regions is found to shift like a seesaw according to variations in the MJO category. In category A, it is found that there is significantly low frequency in the number of geneses in the two bottom quadrants during summer and JJ, but not during AS (Figs. 4a, 4e and 4i). As the category changes from A to B (cf. Figs. 4a and 4b), the number of TCs in the southwest quadrant during summer changes from 6, which is significantly below normal, to 21, which is neither significantly below nor above normal. A change in this quadrant mostly accounts for that in the entire domain (48 versus 65). This significant increase is also found during both JJ (2→11, cf. Figs. 4e and 4f) and AS (4→10, cf. Figs. 4i and 4j). Although changes in the actual number are not as large as those in the southwest quadrant, other notable changes in the number from A to B are found in two top quadrants: the number in the northwest quadrant becomes significantly below normal in category B, but significantly above normal in the northeast quadrant. As the category changes from B to C (cf. Figs. 4b and 4c), a significant increase in the number of TC geneses is observed in both the northwest (9→23) and southeast quadrants (13→28), but a decrease (22→10) in the northeast quadrant; this is associated with enhanced convection activity and the circulation response in the WNP (Figs. 2c, 5c and 6c). The significant variations are also seen in the northeast (8→1) and southeast (4→14) quadrants during JJ (cf. Figs. 4f and 4g), and in the northwest (5→12) and southwest (10→6) quadrants during AS (cf. Figs. 4j and 4k). For the changes from category C to D (cf. Figs. 4c, 4g, 4k and 4d, 4h, 4l), the overall genesis locations shift northward, especially in the west of the mean genesis longitude; this is associated with the intrusion of a reduced convective phase into the tropical western Pacific (Fig. 2d). However, the statistical significance of the northward shift is only found in the northwest quadrant (12→18) during AS (Fig. 4l).
The dynamic parameters that control TC genesis, such as the 850-hPa relative vorticity (Fig. 5) and total and zonal vertical wind shear (Fig. 6), were investigated with respect to each MJO category. Consistent with the northward propagation of the MJO-related convection center, as seen in Fig. 2, the 850-hPa vorticity anomalies move north as well (Figs. 5a–d). The propagating characteristics during JJ (Figs. 5e–h) and AS (Figs. 5i–l) are nearly identical to those during summer. In categories A and B, quite a few TCs form to the northeast of the negative vorticity anomalies. TC genesis increases along the periphery of the equatorial positive vorticity anomalies in category B. The concentration of TC genesis over the positive vorticity anomalies dramatically increases in categories C and D, indicating that many of TC geneses are systematically linked with the propagation of the MJO. While not shown in the figure, the increase of positive vorticity anomalies is related to an enhanced monsoon confluent zone due to an increase in low-level westerlies. In this mean state, favorable conditions for TC genesis occur over the confluence region possibly through the wave accumulation (e.g., Maloney and Hartmann 2001; Kuo et al. 2001; Aiyyer and Molinari 2003) and/or the emanation of Rossby waves in the wake of a preexisting TC (e.g., Sobel and Bretherton 1999; Li et al. 2003; Li and Fu 2006).
As the MJO convection center migrates from the Indian Ocean to the WNP, the spatial field of vertical wind shear indicates the intrusion of a strong shear zone into the tropical WNP, with easterlies to the west and westerlies to the east (cf. Figs. 6a, 6e, 6i and 6c, 6g and 6k). While the intrusion of the easterly shear mainly occurs between the equator and 15°N, that of the westerly shear is centered between 10° and 20°N. The intrusion of the strong shear zone makes the weak shear region (<15 m s−1) narrower, causing a more spatially clustered TC genesis within the region. For instance, the weak shear region covers a vast area of the WNP in category A, resulting in the spread of TC genesis locations (Figs. 6a, 6e and 6i). On the other hand, it becomes much narrower in both zonal and meridional directions in category C, resulting in the clustered TC genesis (Figs. 6c, 6g and 6k). In contrast to JJ, the intrusion of the easterly shear zone becomes broader during AS so that the westerly shear zone to the east becomes narrower. Further, it is found that TCs prefer to form in regions of weak easterly vertical wind shear, especially in categories C and D in which the active MJO-related convection and corresponding enhanced cyclonic vorticity are propagating in the WNP (Frank and Roundy 2006). However, this propensity disappears during the suppressed convective periods of the MJO in the WNP, that is, categories A and B.
Tropical cyclone tracks generally follow the steering flows, defined as the tropospheric layer-mean winds (Chan and Gray 1982), around the periphery of a subtropical high. Hence, it is expected that the geographical distribution of TC tracks would be influenced by systematic changes in the steering flows linked to the phase transition of the MJO. Figure 7 shows actual TC tracks during summer (Figs. 7a–d), JJ (Figs. 7e–h), and AS (Figs. 7i–l) for each MJO category and the climatologies and anomalies of the TPF are given in Fig. 8. In addition, the total fields of the tropospheric layer-mean winds (i.e., steering flows) and their statistically significant anomalies by a two-tailed t test for each MJO category, along with the statistically significant regions of the 500-hPa geopotential height, are presented in Fig. 9.
In the case of category A, straight-moving TCs to the South China Sea are relatively few and nearly half of the TCs that formed in the WNP pass across the ocean southeast ocean of Japan (Figs. 7a, 7e and 7i). These characteristics are clearly observed in the TPF plot: the TPFs increase over the ocean southeast of Japan, but decrease over the Philippine Sea and toward the South China Sea and Korea (Figs. 8b, 8g and 8l). The increase southeast of Japan is statistically significant over the 90% confidence level. The large-scale circulation involves two anticyclonic anomalies impinging against a cyclone between them: one along the South China Sea toward the Philippine Sea and the other offshore east of Japan (Figs. 9a, 9e and 9i). While the two anticyclonic anomalies expand the domain of the WNP subtropical high (WNPSH) to the South China Sea and offshore east of Japan, the cyclonic anomaly between them weakens the strength of the WNPSH south of Japan. If we consider these wave responses in the steering flow together with the genesis parameters that were shown in Figs. 5 and 6, we can reason that the MJO-related variability in TC tracks in this category is largely influenced by the genesis region at a first order. The northward propagation of the TCs that formed around the southern part of the cyclonic anomaly is mainly due to the weakened WNPSH offshore south of Japan. On the other hand, the relatively weak TC activity over the Philippine Sea toward the South China Sea is mainly caused by fewer TC geneses there due to suppressed convection (Figs. 2a and 4a).
In the case of category B, the frequency of straight-moving TCs is obviously greater compared to that of category A (Figs. 7b, 7f and 7j). This difference between the two categories is mainly due to a considerable increase in the number of geneses in the southwest quadrant (Figs. 4b, 4f and 4j). The TCs formed in the southwest quadrant, that is, the southern periphery of the WNPSH, are steered by the easterlies (Figs. 9b, 9f and 9j) so that they tend to propagate straight to the west. This results in an increase of the TPF to the west of the main formation region (Figs. 8c, 8h and 8m). Compared to JJ, however, there exists an eastward shift in the positive TPF region during AS, which is caused by the conglomerate of TC geneses around 150°E in the southeast quadrant (Fig. 4j) and their northwestward propagation over the region of enhanced easterly steering flows (Fig. 9j). The strengthening of the WNPSH around the East China Sea is attributed to a northward migration of the anticyclonic anomaly, especially apparent during AS, resulting in a decrease of the TPF anomalies along the East China Sea through the east Philippine Sea.
In the case of category C, the overall density of TC tracks increases owing to the increase in the number of geneses (cf. Figs. 7c, 7g, 7k and 8d, 8i, 8n). The increase is statistically significant along the Philippine Sea–East China Sea–Korea, which may be due to the increase in the number of geneses in the northwest and southeast quadrants, as shown in Fig. 4. In this category, the strong westerly wind bursts along the equator alter the large-scale monsoon circulation, enhancing the monsoon trough (Figs. 9c, 9g and 9k). As a result, an anomalous cyclonic cell dominates along the South China Sea and across the Philippine Sea during both JJ and AS. There is another anomalous cyclonic cell far offshore southeast of Japan, showing a large seasonal difference: it is located around (20°N, 160°E) during JJ that is a slightly southeast position from the center of the WNPSH and is located around (35°N, 160°E) with stronger intensity during AS that is a northeast position from the center of the WNPSH. The latter represents a strong midlatitude trough (Fig. 9k) that is related to several northward-propagating tracks (Fig. 7k) over that region. Meanwhile, the TCs formed offshore east of the Philippines show slightly more north-oriented tracks, compared to category B. This is also apparent in Fig. 8d, in which the region of increased TPF shifts slightly northeastward. This more north-oriented steering of TCs is related to the weakened easterly steering flows around the Philippines caused by the expansion of the monsoon trough. Also, this is apparently inferred from the strong anomalous westerlies south of 15°N, which may block the westward propagation of the TCs formed over the Philippine Sea.
Category D also shows dense tracks over the northwest Philippine Sea toward the East China Sea; however, the density of tracks offshore east of the Philippines toward the South China Sea is slightly lower (cf. Figs. 7d, 7h, 7l and 8e, 8j, 8o). The reasons for this variability are as follows. First, TC genesis decreases in the two southern quadrants (Figs. 4d, 4h and 4l). Second, the westerly anomalies propagate west of 140°E in the region 10°–20°N in association with the northward-propagating cyclonic anomaly; the westerly anomalies are then altered to become southerly anomalies offshore south of Japan as they meet the easterly anomalies, which makes the WNPSH retreat to the east, but strengthen it meridionally (Figs. 9d, 9h and 9l).
To provide more detail, TC tracks are plotted separately within the four quadrants divided according to subseasons (JJ and AS) (Fig. 10). The TC tracks that formed in the northeast quadrant for the four MJO categories are displayed in Figs. 10a–d. The distinction between tracks of category A and the others is noticeable; the TC tracks of category A are concentrated offshore southeast of Japan, compared to those of other categories. This means that the TCs formed in the northeast quadrant are steered more systematically in category A than in other categories. The TC tracks of categories B, C, and D, by contrast, show a sporadic distribution.
Next, the TCs originating from the northwest quadrant are presented (Figs. 10e–h). On the whole, the movement in this quadrant looks erratic, which may be due to variable steering. The TCs formed during JJ preferably propagate westward due to the effect of the strong ridge in categories A and B (Figs. 9e and 9f), but their direction of propagation becomes erratic due to the weakening of the WNPSH there in categories C and D (Figs. 9g and 9h). Also, tracks propagating westward are dominant in category B, but those propagating northward are more numerous in category D according to the intensity variations of the WNPSH in that region (Figs. 9b and 9d).
It should be noted that TC activity in the southwest quadrant is revealed to be very sensitive to the MJO (Figs. 10i–l). In addition to variations in the number of geneses, the TC tracks are more westward oriented in categories A and B (Figs. 10i–j), while they are slightly northward oriented in the cases of categories C and D (Figs. 10k and 10l). These features are easily understood by examining the steering flows around the periphery of the WNPSH in this quadrant, in which the easterlies are weakened by the intrusion of the MJO-related westerly wind bursts along the equator between categories B and C (see Figs. 9j and 9k). Owing to more northward-oriented tracks in category C, some TCs can reach the East China Sea, and further reach the land on the Korean peninsula. The seasonal difference between JJ and AS is negligible.
Finally, we plot the TCs formed in the southeast quadrant (Figs. 10m–p). Together with the TCs of category A in the northeast quadrant, those of category A in this quadrant also contribute significantly to an increase in the TPF southeast of Japan (Fig. 10m). The weakened ridge north of the region lets the TCs propagate northward (Fig. 9i). In contrast to the variability in the northeast quadrant, the TCs of category B propagate more to the west than those of category A, that is, they are well clustered compared to the TCs of other categories (Fig. 10n). This is because the WNPSH in category B is stronger than that in category A (Fig. 9j). In categories B and C, there exists a noticeable seasonal difference in TC tracks, with more straight-moving TCs during JJ than during AS. This is obviously due to the difference of the mean location of the western periphery of the WNPSH (cf. Figs. 9f, 9g and 9j, 9k). However, the tracks in category D do not show any remarkable seasonal difference.
c. Landfalling statistics
In this study, the coastal area is divided into seven subareas: the Philippines, Vietnam, south China, Taiwan, east China, Korea, and Japan (Fig. 11). The main factor taken into account is the national boundary, but China is further divided into two subdivisions (i.e., south China and east China) with respect to an artificial boundary line along 25°N due to its large territory.
Table 2 gives the statistics for the number of days and TC landfalls for the four active MJO categories, and the category NONE (weak MJO activity period), with respect to each subarea. From a statistical perspective, there is a significant modulation in Vietnam, south China, Korea, and Japan over the 90% confidence level using a two-tailed t test. Variations in the remaining three subareas also exhibit a modulation by the MJO to some degree, but they are not significant at the 90% confidence level. However, defining the landfall from the best-track dataset is a subtle skill because some tracks are not easy for us to decide whether they cross the coastal line or not. After testing the number of landfalls by slightly changing the extent of the landmass area, a robust and statistically significant signal was found in south China, Korea, and Japan.
While it is not statistically significant, the number of TC landfalls in the Philippines slightly increases to 14 (2.7% of the total of 513 days for category B) and 13 (2.6% of the total of 506 days for category C) for categories B and C, respectively, compared to the climatology (2.2% of the total of 3172 days). This is obvious because of frequent TC geneses offshore east of the Philippines (see Figs. 4b and 4c). Vietnam in category A experienced only four TCs (0.8% of the total of 530 days for category A); this number is statistically significant at the 90% confidence level. The number increases to 13 (2.5%) for category B, to which the major contributing factors are an increase in the number of straight-moving TCs propagating into the South China Sea across the Philippines that formed in the offshore area east of the Philippines as well as frequent genesis in the South China Sea. In the south China area, there is a robust and statistically significant modulation in categories A and C; this is consistent with the variability of convection and the large-scale steering flows (cf. Figs. 2a, 9a and 2c, 9c).
In Taiwan, the number of landfalling TCs is slightly larger for categories C (i.e., 10) and D (i.e., 11) than for categories A (i.e., 7) and B (i.e., 5), but none of them are statistically significant. The modulation in TC landfalls over east China is the weakest. In this area, the number does not show any systematic changes in relation to the MJO. On the other hand, it is found that TC landfalls are strongly concentrated in a specific category in Korea. While Korea experiences only one (0.2%) TC landfall in category A, the number increases to 11 (2.2%) in category C. This signal is the most robust and is unaffected by any changes. All of these values are significant over the 90% confidence level. In particular, the percentage value in category C is significant at the 99% confidence level, compared to the climatology (0.9%). In Japan, the number of TC landfalls is the smallest in category A (i.e, 6), which is statistically significant at the 90% confidence level, and the largest in category D (i.e., 15), which is not statistically significant.
d. Separation of the ENSO effects
As discussed in the introduction, ENSO has been known to be the most outstanding planetary-scale phenomenon affecting interannual variations of TC activity in the WNP. It has been found that the MJO is also related to ENSO warm events (e.g., Kindle and Phoebus 1995; Wang and Weisberg 2000; Bergman et al. 2001; McPhaden 2004). Although the mechanism of the effects of the MJO on ENSO is still a topic of debate, strong MJO events have been frequently observed during the developing stages of recent major El Niño events. Further, Zhang (2005) mentioned that the interannual SST warming in the central and eastern Pacific is comprised several intraseasonal events associated with the MJO. Thus, it is necessary to take the effect of ENSO into account in the present study.
To simplify the problem, ENSO years are chosen based on the Niño-3.4 index. The selected years were described in section 2. Figure 12 displays all TC tracks and the number of geneses and their division by category for El Niño, La Niña, and neutral years. In addition, the statistics of the number of days and TC geneses for each MJO category in relation to ENSO are given in Table 3. The TCs during El Niño (La Niña) years largely form in the southeast (northwest) quadrant (Figs. 12a and 12f), as revealed in many previous studies (e.g., Fudeyasu et al. 2006, and references therein). In accordance with the interannual shift in the major region of genesis, the variability associated with the MJO is highly concentrated in the southeast and northwest quadrants during El Niño and La Niña years, respectively (cf. Figs. 12b–e and 12g–j). Changes in the number of basinwide geneses for ENSO events are similar to those for all years with the concentration of geneses in categories C and D (Table 3). Though extreme ENSO events are removed, spatial variations of TC geneses and tracks are nearly identical to those for all years (Figs. 12l–o). In addition, the variability of the TPF anomalies is well conserved (figure not shown). However, the modulation of the number of basinwide TC geneses (35→40→44→41) becomes slightly weaker, compared to that for El Niño and La Niña years, suggesting the possibility of the intensification of the MJO effect on TC activity during extreme ENSO events. This view needs further substantiation in any future studies.
In the present study, we have explored the systematic variations of summertime TC activity in the WNP in relation to the MJO. By applying a space–time wave filter to the OLR data during 1979–2004, the MJO can be defined as eastward-propagating waves whose wavenumbers range from 0 to 5 and periods from 30 to 90 days. Next, the EOF analysis is performed to define the phase and amplitude of the MJO. The four active MJO categories (A–D) and category NONE indicating periods of weak MJO activity are defined. Based on these defined categories, the TCs are placed into each category and composite maps of the OLR and NCEP–NCAR data are obtained. The categorized TCs are further examined by dividing them into four quadrants (i.e., northeast, northwest, southwest, and southeast) whose center is located at (15.9°N, 138.8°E); this center is the mean genesis position of all summertime TCs. The TC categorizing procedure and composite analyses are repeated for JJ and AS to consider the seasonality. In addition, the effect of strong ENSO events is separated from the TC analyses.
Category A presents the smallest number of TC geneses (i.e., 48) in all categories, which the MJO-related enhanced convection locates in the tropical Indian Ocean. It is manifest in the southwest quadrant where the number is 6; hence, there are very few straight-moving TCs in the South China Sea. However, it shows that TC activity greatly increases in the ocean southeast of Japan; this is attributed to both the intrusion of the weak vertical shear zone in that region and the weakened WNPSH, which results from the cyclonic anomaly between the two significant anticyclonic anomalies: one along the South China Sea across the Philippine Sea and the other offshore east of Japan. The former is directly connected to the MJO-related suppressed convection cell in the South China Sea and the latter may be located along the great circle of the wave train induced by anomalous MJO-related heating. In this category, the number of TC landfalls is statistically significantly decreased in Vietnam, south China, Korea, and Japan compared to climatology.
From categories A to B, the number of TC geneses greatly increases, from 6 to 21, in the southwest quadrant along with the intrusion of a strong convective region to the equatorial western Pacific. Moreover, straight-moving TCs increase to the South China Sea along with the westward expansion of the WNPSH. Meanwhile, the longitudinal zone of weak vertical wind shear becomes narrower, resulting in an intensified degree of clustering in the monsoon confluence zone. This variability is evident during JJ, but not during AS.
Since the anomalous deep convection around the equator migrates farther north and the WNPSH retreats northeastward in category C, a cyclonic circulation anomaly prevails over most of the WNP basin. The weak shear zone becomes further narrowed, especially during JJ. Accordingly, TC genesis is most active (i.e., 81) and is clustered in the region of active convection for this category. In addition, the major genesis region shifts to the north and east (i.e., the northwest and southeast quadrants) with many TC geneses in the southwest quadrant (i.e., 20). However, the number of geneses decreases considerably in the northeast quadrant (22→10). The region of TC geneses in this category is directly linked with the MJO-related enhanced convection. In comparison to category B, more TCs form in the north South China Sea and, further, reach south China; the TPF through the Philippine Sea–east China Sea–Korea line increases, resulting in significantly enhanced TC landfalls in south China and Korea.
The anomalous deep convection moves further northward and is in a decaying stage in category D. Therefore, the overall genesis frequency is slightly reduced when compared to category C and migrates northward. Consistent with the changes in large-scale environments (i.e., the eastward retreat and meridional broadening of the WNPSH), TCs propagate preferentially to the east China Sea and farther to Japan. Consequently, Taiwan and Japan experience a slight, but statistically insignificant, increase in the number of TC landfalls in this category.
Analyses of the ENSO effects reveal that spatial variations of TC activity associated with the MJO during extreme ENSO events are dependent upon the interannual shift in the major genesis location. However, the spatial variations for neutral years have nearly the same magnitude as those for all years, indicating that those are characteristic signals induced by the intraseasonal propagation of the MJO, rather than a merely intraseasonal manifestation of ENSO-related ones.
Intraseasonal variations of the location of TC genesis associated with the MJO are reminiscent of interannual variations associated with ENSO. While the latter shows a northwest–southeast oriented axis of variations in terms of the location of TC genesis (see Figs. 12a and 12f), the former shows a seesawlike moving axis (see Fig. 4). On this score, variations of TC genesis associated with the MJO differ from those associated with ENSO.
East–west oriented variations of the density of TC tracks appear on an interannual time scale associated with ENSO as well as on an intraseasonal time scale associated with the MJO, especially during JJ and autumn (Wu and Wang 2004; Fudeyasu et al. 2006). However, the variations associated with ENSO are less clear than those associated with the MJO during AS (Fudeyasu et al. 2006).
A remarkable contrast is revealed in terms of the statistics of TC landfalls. Deterministic large-scale steering circulations that control TC landfall in Korea and Japan are induced by the MJO rather than by ENSO, seeing that a robust and significant modulation in the number of TC landfalls is observed in Korea, rather weakly, and also in Japan, but is not observed in landfalling statistics associated with ENSO. Interannual variations of the number of TC landfalls in Korea and Japan may be better controlled by those of the zonally oriented quasi-stationary Rossby wave train along the summer-mean jet stream than by ENSO (Kim et al. 2005b).
Systematic variations in the degree of clustering of TC tracks according to the MJO category is associated with the monsoon trough–WNPSH covariability on an intraseasonal time scale, which was presented in Harr and Elsberry (1991, 1995). As illustrated in Figs. 2 and 9, the northward propagation of MJO-related convection and circulation anomalies in the monsoon trough region possibly influences the outer trough region by Rossby wave emanation such that the WNPSH may expand or shrink; this leads to distinct TC tracks and landfalls divided on the basis of the four MJO categories, as discussed in section 3.
Although we have not discussed the period of weak MJO activity (category NONE) in detail, it contributes a significant portion of the total number of TC geneses as well as the landfalling statistics (e.g., Fig. 4 and Table 2), suggesting that the MJO is merely one modulating factor among many factors with different space and time scales. In this regard, one of the conclusions of Liebmann et al. (1994) is appropriate—that TC activity is also modulated by an intraseasonal variability that is a completely independent band from the MJO. This other intraseasonal variability may be related to the submonthly oscillation, which may consist of a 10–25-day intraseasonal oscillation (e.g., Fukutomi and Yasunari 1999) and several known tropical waves such as the equatorial Rossby waves, MRG waves, TD-type waves, and so on (e.g., Lau and Lau 1990; Takayabu and Nitta 1993; Wheeler and Kiladis 1999; Frank and Roundy 2006). The latter waves having higher frequencies and westward-propagating properties are found to be closely related to variations of TC activity (e.g., Chang et al. 1996; Dickinson and Molinari 2002; Bessafi and Wheeler 2006; Frank and Roundy 2006).
Clustering of TC genesis within the MJO-related convective region is observed when the MJO-related convection center is found in the WNP. This introduces a probable hypothesis that there are more chances of TCs being generated by means of Rossby wave dispersion in the wake of a preexisting TC (e.g., Sobel and Bretherton 1999; Li et al. 2003; Li and Fu 2006). One case that may support this hypothesis is the TC activity in June 2004, during which there were five successive TC geneses within the strong MJO convective envelope (Kim et al. 2005a; Nakazawa 2006). Further studies are necessary to prove this hypothesis.
Another important issue is that these higher-frequency signals also interact with the larger space-scale and longer time-scale variability, such as the MJO (e.g., Matthews and Kiladis 1999; Straub and Kiladis 2003). As noted in Straub and Kiladis (2003), there are evidently periods when this mechanism is activated. From this viewpoint, nonlinear scale interaction processes within monsoon environments, as discussed by Holland (1995), are insightful. The results of this study may also implicitly suggest this issue. Based on the fact that there are a large number of TCs in each MJO category, the signal of TCs may also contribute a significant portion of the intraseasonal convection and circulation behavior. In other words, scale interaction is the most critical function for summertime climate variability in the WNP.
This study was funded by the Korea Meteorological Administration Research and Development Program under Grant CATER 2006–4204. JHK and HSK were also supported by the Brain Korea 21 (BK21) Project in 2007. CHS was supported by the National Sciences Council in Taiwan under Grants NSC 093-2111-M-008-002 and NSC 094-2111-M-008-008. Part of this work was carried out by JHK in Taiwan during the period of 1 March 2005–31 March 2006 and was supported by the same NSC grants. The authors are grateful to three anonymous reviewers. Their helpful comments and suggestions led this study to a publishable work.
Corresponding author address: Chang-Hoi Ho, Climate Physics Laboratory, School of Earth and Environmental Sciences, Seoul National University, Shillim-dong, Gwanak-gu, Seoul 151-742, Korea. Email: firstname.lastname@example.org