Analysis of the Anomalous Signals near the Tropopause before the Overshooting Convective System Onset over the Tibetan Plateau

(is study investigates the anomalous signals near the tropopause before the overshooting convective system (OCS) onset over the Tibetan Plateau (TP). It is found that the tropopause height is stable at the maximum height for the 7th day and the 5th day before the OCS onset. It then decreases significantly one day before and on the day of the OCS onset. (e upward motion in the troposphere is the strongest for the 5th day before the OCS onset. From one day before and after the OCS onset, there are strong ascending motions at 500–300 hPa but weak descending motions near the tropopause. It is proposed that the descending of the tropopause height on the day of the OCS onset is caused by frequent tropopause fold events over the eastern TP associated with frequent cold trough intrusion from the north and the southeastward movement of upper-level westerly jet stream. (e decrease of the tropopause height is accompanied by the intrusion of stratospheric air with higher potential vorticity (PV). Positive potential vorticity anomalies on 350K isentropic surface can be noted in the region where the tropopause height decreases one day before and on the day of the OCS onset. With the deepening of the tropopause fold on the day of the OCS onset, there is not only downward motion near the tropopause in the area behind of the fold but also upward motion in the troposphere beneath the folding region. In addition, the upward displacement of isentropic surfaces leads to an upper-level cold pool, which causes a reduction in static stability beneath the PV anomaly on the day of the OCS onset. (e upper-level PV anomalies and their associated strong instability in the middle troposphere can trigger convective activities by the release of potential instability on the day of the OCS onset. (e overshooting convection is more likely to occur due to lower tropopause height, although upward motion in the troposphere is not the strongest.


Introduction
e deep convection can effectively redistribute trace gases throughout the atmosphere by changing the trace gas composition and thus plays an important role in the stratosphere-troposphere exchange (STE) [1][2][3]. Observational evidences show that deep convection at high altitude can be strong enough to penetrate the tropopause and rise into the stratosphere (hereinafter referred to as overshooting convective system (OCS)), which directly injects water vapor, pollutants, and even ice crystals into the stratosphere [4,5]. Recently, Sang et al. [6] proposed that overshooting convective activities increase water content in the lower stratosphere, which is a result of the sublimation of ice crystals that pass through the tropopause and mix with the warmer stratospheric air. e increase in the stratospheric water vapor can intensify the global greenhouse forcing [7] and enhance ozone depletion [8,9], which will subsequently affect the radiation budget and surface temperature [10].
Luo et al. [25] conducted a comprehensive study on deep convection over different regions of the Tibetan Plateau--Asian monsoon region and showed that the cloud tops over the TP are more densely packed than the other subregions. Qie et al. [2] found that deep convective systems with 20 dBZ echo tops exceeding 14 km occur frequently over the TP. Heath and Fuelberg [26] defined convective trajectories as those that started at the upper-level anticyclone and reached the top of the boundary layer at some time during their 6 h back track, and they revealed that more than 90% of convective trajectories originated in the TP and the southern slope of the Himalayas at both 100 and 150 hPa. On the other hand, the STE associated with the tropopause folds accounts for a large proportion of total STE over the TP [27,28]. Tropopause folds can cause stratospheric air to be transported downwards to the atmospheric boundary layer and influence the vertical distribution of tropospheric greenhouse gases such as ozone over the TP [27][28][29]. Because tropopause folds are associated with development of upperlevel positive potential vorticity (PV) anomalies, they could possibly contribute to rapid cyclogenesis, deep convective storms, and other severe weather events [30,31]. Considerable progress has been made in understanding the formation of deep convection over the TP. e complex terrain and unique thermal and dynamical forcing of the TP make it an active region of strong summer convective systems [18,22]. As the low-level layer of warm and moist air from the Arabian Sea and the Bay of Bengal over the Indian subcontinent is obstructed by the steep mountain barrier, it is capped by an elevated layer of dry air advected off the Iranian or Tibetan Plateaus. e capped low-level monsoon airflow accumulates instability via surface heating over the TP [32,33]. Furthermore, the westerly jet stream moves to northern TP in summer from the southern TP in winter. e lee side of the Tibetan Plateau has been identified as one of the two maxima for the development of baroclinic disturbances and cyclogenesis in the extratropical Northern Hemisphere, which is beneficial to the occurrence of synoptic-scale weather systems [34]. Nevertheless, the mechanism for the formation of overshooting convective systems over the TP has not been fully understood yet.
Traditionally, the stratosphere is considered to be a passive layer that is affected by the troposphere, and it has little influence on the surface weather systems. However, the circulation regimes in the stratosphere tend to persist for several weeks or longer. Observations suggest that large stratospheric anomalies can be used as a predictor of tropospheric weather patterns [35][36][37][38][39]. Hartley et al. [40] and Black [41] found that anomalous changes in stratospheric potential vorticity (PV) can induce perturbations in key meteorological fields in the upper troposphere and thus have important influences on synoptic systems in the troposphere. Colucci [38] proposed that the midtropospheric anticyclogenesis associated with the blocking case critically depends on the stratospheric contribution and should not be solely explained by tropospheric processes. Luo et al. [42] found that the Northern Hemisphere Annular Mode (NAM) index near the tropopause region is one of the good factors for forecasting precipitation in the Meiyu season. At present, results of numerical models also indicate that the tropospheric weather systems can be better simulated when the representations of the stratosphere and stratospheric processes are improved in models [43][44][45][46]. It can be seen that an improved understanding of the dynamical link between the stratosphere and the troposphere is expected to lead to improved confidence in both long-range weather forecasts and climate change projections [47].
However, the anomalous signals around the tropopause and in the stratosphere before the onset of the overshooting convective system over the TP have not been fully analyzed in previous studies. e present study aims to investigate temporal and spatial variations of the tropopause height, the potential vorticity, and meteorological fields before the overshooting convective systems onset and to find out the anomalous signals in the tropopause and lower stratosphere before the overshooting convective systems onset over the Tibetan Plateau. is paper is organized as follows. Section 2 describes the data and method used in this study. Section 3 presents the results. Summary and discussion are given in Section 4.

Data and Methods
e characteristics of convective systems are identified based on the 16 yr period (1998-2013) of Tropical Rainfall Measuring Mission (TRMM) radar precipitation feature (PF) level 2 data downloaded from the University of Utah database [48]. e method to define radar PFs by grouping the area of ground projection of radar reflectivity greater than or equal to 20 dBZ is adopted in the present study [48,49]. However, the data for August 2001, when the TRMM satellite's orbit was boosted to lengthen its mission, are excluded due to concerns of the data quality and reliability during this period [50]. As the first quantitative spaceborne radar, the TRMM precipitation radar (PR) provides 3D structural features of precipitation systems. e TRMM PR has horizontal resolutions of 4.3 km (before the orbit boost in August 2001) and 5 km (after the boost). It has a 215 km swath width that extends from the surface to 20 km above the Earth ellipsoid with the vertical resolution of 250 m [49]. e erroneous TRMM PF cases described by Qie et al. [2] are excluded.
e TRMM PF dataset is used to identify deep convective systems reaching above the tropopause height. e maximum height of 20 dBZ radar echo (Maxht20) is an indicator of the PF depth [51,52]. e reference height to define overshooting convective system (OCS) is determined according to WMO lapse rate tropopause height definition [53] in this study, which is defined as the lowest level at which the lapse rate decreases to 2 K km −1 or less, provided that the average lapse rate remains less than 2 K km −1 for 2 km above this level. is is also one of the methods used by Liu and Liu [54]. Several previous studies have demonstrated that the lapse rate tropopause height derived from the ERA-Interim analysis is suitable for such efforts [55]. In this study, we use the 0.25°× 0.25°, 6-hourly ERA5 reanalysis data with better spatial and temporal resolution, which allows for a better representation of convective updrafts, gravity waves, tropical cyclones, and other meso-to synoptic-scale features of the atmosphere [56]. Because the ERA5 analyses of lower stratospheric temperature exhibit a pronounced cold bias from the years 2000-2006 [57], we replace the temperature using 0.25°× 0.25°, 6-hourly ERA5.1 reanalysis with better global-mean temperatures in the stratosphere and uppermost troposphere during 2000-2006. First, the lapse rate tropopause height derived 0.25°× 0.25°, 6-hourly ERA5 and ERA5.1 data are temporally and spatially interpolated to the time and location of each PF. Second, the vertical profile for each PF is interpolated into 0.1 km intervals to calculate the lapse rate tropopause height according to the WMO definition. en, the overshooting convective systems are defined by TRMM PFs with Maxht20 reaching above the lapse rate tropopause height. In total, 41 OCS events are found over the TP in the summers (June, July, and August) during 1998-2013. e detail dates about 41 OCS events are listed in Table 1. Figure 1(a) shows geographical locations of the 41 OCS events in summer over the TP based on 16 years of TRMM observations. We can note that the OCS events are mainly found over the eastern TP from Figure 1(a). e scatter plot of Maxht20 and tropopause height derived from 41 OCS events are shown in Figure 1(b); the average values of Maxht20 and tropopause height are 17.28 km and 16.78 km above the sea level, respectively.
A composite analysis is performed with respect to days before and after the onset of OCS events. Note that all the meteorological fields, including tropopause height, potential vorticity, temperature, zonal and meridional winds, geopotential height, and vertical velocity, are temporally and spatially interpolated to the time and location of 41 OCS using 0.25°× 0.25°, 6-hourly ERA5 and ERA5.1 reanalysis data. e composite field on the nth day before (or after) the onset of OCS events is the average of the specific field on the nth day for 41 OCS events. e nth day before (after) the occurrence of OCS event is recorded as time = −n (+n)th day, and the day of the OCS occurrence is recorded as time = 0 day. e anomalies presented in this study are computed as deviations from the daily climatological annual cycle during 1998-2013. A two-sided Student's t-test is used to assess statistical significance. Figure 2(a) shows the composite time series of anomalous dynamic tropopause height and tropopause temperature from the 15th day before to the 5th day after the OCS onset derived from ERA5 and ERA5.1 reanalysis data with the high resolution (0.25°× 0.25°) averaged for 41 OCS events. e dynamic tropopause height is estimated from the PV field using a 3.5 potential vorticity unit (PVU) threshold (1 PVU = 10 −6 ·m 2 ·K·kg −1 ·s −1 ). It is evident that the tropopause height rises rapidly from the time = −14th day to −11th day. It then decreases slightly from the time = −11th day to −10th day. e tropopause height reaches the maximum height at the time = −7th day and −5th day. It then descends significantly from the time = −5th day to −1st day, followed by a small fluctuation in the tropopause height between the time = −1st day and 0 day. e difference of tropopause height between the time = −5th day and the time = −1st day can reach 0.21 km. e tropopause height ascends after the OCS onset. e variation of tropopause temperature is consistent with the tropopause height, except that the tropopause temperature is abnormally high on the day of OCS onset. Figure 2(b) shows the composite evolution of time-pressure cross sections of vertical velocity from the 15th day before to the 5th day after the onsets of OCS averaged for 41 OCS events. Note that there are weak descending motions in the lower stratosphere and upper troposphere when the weak descending of tropopause height occurs near the time = −9th day. From the time = −6th day to −1st day, the ascending motions are found at 500-150 hPa in the troposphere. At the time = −5th day, the upward motion in the troposphere is the strongest, which can reach near the tropopause when the maximum positive anomaly of tropopause height occurs, corresponding to highest tropopause height. From the time = −1st day to 1st day, there are strong ascending motions at 500-300 hPa but weak descending motions near the tropopause (Figure 2(b)). We can note that the change in tropopause height accompanying OCS is closely related with the evolution of vertical velocity, and the overshooting convection does not occur when the upward motion in the upper troposphere is strong due to the higher tropopause height at the time = −5th day. However, the overshooting convection occurs when the tropopause height is lowered at the time = 0 day. To show the details of anomalous tropopause height pattern before the onsets of the OCS events, the composite horizontal distributions of tropopause height anomalies at the time = −7th, −6th, −5th, −4th, −3rd, −2nd, −1st, and 0 day for 41 OCS events are shown in Figure 3. Note that significant variation of the tropopause height before the onsets of the OCS events occurs over the eastern TP. e tropopause height over the eastern TP is significantly strong positive anomaly from the time = −7th day to −4th day (Figures 3(a)-3(d)). e positive anomaly of tropopause height over the east of TP slightly decreases from the time = −3rd day to −2nd day (Figures 3(e)-3(f )). At the time = −1st day and 0 day, the tropopause height becomes significantly negative anomaly at the longitude range of 96°-100°E (Figures 3(g)-3(h)). is is consistent with the descending of tropopause height between the time = −1st day and 0 day shown in Figure 2(a). Chen et al. [28] indicated that the interaction occurred between deep convective boundary layer and the low tropopause over the TP,   and convection was a central player in cases of the high convective boundary layer. Griffiths et al. [31] also proposed that there is a dynamical link between the lowered tropopause and convection. erefore, the decrease of the tropopause height at the time = −1st day and 0 day may be related to the occurrence of OCS. Chen et al. [58] demonstrated that variations in the height of the tropopause were related to tropopause folds. It is likely that the decrease in tropopause height at the time = −1st day and 0 day in Figures 2(a) and 3 results from a tropopause fold event. In the next section, the characteristics of tropopause fold are analyzed.

Potential
Vorticity. e dynamical role of the tropopause can be determined using the PV concepts. In order to understand the possible mechanism of descending of tropopause height accompanying the OCS events, Figure 4 shows the composite horizontal distribution of PV anomalies on 350 K isentropic surface at the time = −7th, −6th, −5th, −4th, −3rd, −2nd, −1st, and 0 day. From the time = −7th day to −4th day before the OCS onset, large negative anomalies of PV on 350 K isentropic surface are found over the eastern TP (Figures 4(a)-4(d)), which are consistent with the strong positive anomalies of the tropopause height (Figures 4(a)-4(d)). e lower PV in the upper troposphere suggests upward transport of air mass over the eastern TP. After the time = −3rd day, the negative anomalies of PV on 350 K isentropic surface gradually weaken (Figures 4(e) and 4(f )), and the PV values on 350 K isentropic surface become strong positive anomaly at 96°-100°E at the time = −1st day and 0 day (Figures 4(g) and  4(h)). e positive PV anomalies on 350 K isentropic surface at 96°-100°E in Figures 4(g) and 4(h) are related with the descending of tropopause height shown in Figures 3(g) and   3(h). It is possible that stratospheric air with higher PV values invades into the troposphere and accumulates, leading to a decrease in the tropopause height. is is in agreement with mechanisms proposed by Chen et al. [28]. e composites of longitude-pressure cross sections at 34°N and latitude-pressure cross section at 98°E of PV and potential temperature at the time = −7th, −6th, −5th, −4th, −3rd, −2nd, −1st, and 0 day for 41 OCS events are shown in Figure 5. Previous studies have shown that the PV values ranging from 1 to 3 PVU can qualitatively delineate the tropopause location based on sounding and aircraft data [59,60]. From the time = −7th day to −2nd day, the PV is higher in the stratosphere and lower in the troposphere, and the change of the tropopause height is very little (Figures 5(a)-5(f )). It is worth noting that there is tropopause depression, and a high PV center (1.5-2.0 PVU) near the 300-200 hPa locates at around 96°-99°E at the time = −1st day ( Figure 5(g)). e tropopause fold structure is evident at the time = 0 day, with the tongue of the tropopause fold located at 96°−99°E, and the stratospheric air with higher PV values extends deep into the troposphere at a height of about 300 hPa ( Figure 5(h)). From Figures 5(g1)-5(h1), the dynamical tropopause also exhibits a folded structure at 32.5°-34°N. ese results are consistent with the distribution of tropopause height displayed in Figure 2(a), which show that the tropopause height reaches its minimum value at the time = −1st day and 0 day. Figures 4 and 5 suggest that a tropopause fold event does indeed occur at 96°-99°E at the time = −1th day and 0 day, and the descending of the tropopause height accompanying OCS onset at 96°-99°E is caused by tropopause fold events.
Previous studies have shown that the tropopause fold with a medium intensity occurs frequently over the TP in the summer with a high value center located near 92°-97°E over the eastern TP [61]. Due to the high occurrence frequency of  Advances in Meteorology the tropopause fold, stratospheric intrusion should frequently happen over the eastern TP, which makes important contributions to downward transport of the stratospheric air with higher PV to the troposphere [62][63][64][65][66][67][68][69][70]. Figures 4 and 5 suggest that a tropopause fold event does indeed occur over the eastern TP and results in obvious upper-level PV anomaly at the time = −1st day and 0 day. Hoskins et al. [71] and Russell et al. [72] proposed that upper-level PV anomalies can reduce convective stability in the troposphere. From Figure 1(a), we can see that the overshooting convective systems in this study also occur mainly over the eastern TP. is intrusion of high PV air may be the result of the latent-heat release at the time = 0 day. It is possible that the descending of the tropopause height caused by frequent tropopause fold events over the eastern TP at the time = 0 day is beneficial to the occurrence of OCS.

Wind
Fields. An analysis of the geopotential height fields and wind fields at dynamic tropopause height (3.5 PVU surface) at the time = −5th, −4th, −3rd, −2nd, −1st and 0 day ( Figure 6) reveals that the tropopause fold event is associated with a cold air trough over the east of the TP, with its western flank extending southeastward into the south of the TP at the time = −4th day ( Figure. 6(b)).
is low pressure trough moves southeastward and deepens, forming a low pressure center at around (25°N, 105°E) at the time = −2nd day (Figure 6(d)). From the time = −1st day to 0 day, the low pressure center disappears and the low pressure trough becomes east-west, and a high pressure ridge locates over the eastern TP (Figures 6(e) and 6(f )). e composited zonal wind speed fields indicate that an upper-level westerly jet stream at 3.5 PVU surface develops at the time = −5th day (Figure 6(a)) and enhances with a jet stream center located over the northern TP at the time = −4th day (Figure 6(b)). In accordance with the movement of the pressure trough, the westerly jet stream intensifies and moves eastward to the northeastern TP from the time = −3rd day to 0 day (Figures 6(c)-6(f )). At the same time, the anticyclone circulation over the western TP also moves eastward from the time = −5th day to −1st day (Figures 6(a)-6(e)). On the day of OCS onset, the anticyclone circulation center moves to the eastern TP ( Figure. 6(f )). It is apparent that the upper-level jet stream, a typical synoptic system related to the formation of the tropopause fold event, is forced by the geostrophic adjustment process associated with the cold air trough. Previous studies have shown that in order to maintain the heat-forming balance, a secondary circulation will be triggered in the vicinity of the upper-level jet stream so that the tropopause is folded downward along the sinking branch of the secondary circulation [73,74]. is is one of the main mechanisms for the formation of the tropopause fold. Figure 7 shows the horizontal distribution of vertical velocity on 350 K isentropic surface from the 7th day to 0 day before the OCS onset for 41 OCS events. Note that the ascending motion on 350 K surface is the strongest at the time = −5th day (Figure 7(c)), resulting in the highest tropopause height shown in Figure 2(a). It is apparent from Figure 7(h) that the area where the tropopause fold is located is accompanied by weak ascending motion at 95°-98°E, while the sinking motion is located to the east of 98°E at the time = 0 day. e most striking feature in Figures 8(e)-8(h) is that the vertical velocity on 350 K isentropic surface appears alternately between the positive and negative centers from the time = −3rd day to 0 day. Previous study found that the forcing terms of the omega and geopotential tendency equation mark the genesis of the extratropical cyclones on the storm track, and they have a maximum value on the lee  Advances in Meteorology side of the TP [34]. It also corresponds to a region of baroclinic development [34]. So the upward movements are intensified through baroclinic processes in this region. Figure 8 shows the composites of longitude-pressure cross sections of vertical velocity and potential temperature at 34°N at the 7th, 6th, 5th, 4th, 3rd, 2nd, 1st, and 0 day before the OCS onset for OCS events. From the time = −3rd day to −2nd day, there are weak ascending motions at 96°-98.5°E and descending motions to the west of 96°E and east of 98.5°E in the troposphere (Figures 9(e) and 9(f )).
fold event occurs, there is not only strong downward transport of air mass from the stratosphere, but also ascending motion in the troposphere beneath the folding region. Moreover, the upward curvature of the isentropic surface in the troposphere associated with a PV anomaly can be seen clearly in the region beneath the tropopause fold from the time = −1st day to 0 day (Figures 8(g)-9(h)). e upward and downward displacements of isentropic surfaces are associated with ascent of tropospheric air beneath the depressed tropopause and descent of air at both sides of the depressed tropopause between the time = −1st day and 0 day. is ascent can contribute to the development of deep  8 Advances in Meteorology convection by releasing potential instability [75]. We can see that the overshooting convection is more likely to occur due to the lower tropopause height, although the upward motion in the troposphere is not the strongest at the time = 0 day.

Static Stability.
e vertical changes of temperature will lead to changes in static stability [76]. Figure 9 shows the composites of longitude-pressure cross sections of temperature and static stability anomaly at 34°N for the 3rd, 2nd, 1st, and 0 day before the OCS onset for OCS events. It is clear that the temperature near the tropopause is a negative anomaly, and the temperature at 700-250 hPa is a positive anomaly at the time = −3rd day (Figure 9(a)), the corresponding static stability in the upper troposphere is weakened (Figure 9(e)). From the time = −1st day to 0 day, the positive anomaly of temperature occurs above the depressed tropopause in the lower stratosphere at around 96.5°-99°E, and the negative anomaly of temperature is strengthened to the west of 96.5°E and the east of 99°E in the lower      d)). e temperature changes on both sides of the depressed tropopause in the lower stratosphere and upper troposphere are more intense at the time = 0 day than that at the time = −1st day. e strong horizontal temperature gradient near the tropopause tends to give rise to tropopause deformation or vertical discontinuity in the thermal tropopause on the day of OCS onset. e increase of temperature in the lower stratosphere at around 96.5°-99°E tends to form a stable layer within the area of tropopause fold, while the decrease of temperature in the troposphere can lead to the decrease of static stability below the depressed tropopause at 700-500 hPa at the time = 0 day (Figure 9(h)).
e change of temperature in the upper troposphere is consistent with the change of isentropic surfaces. Negative temperature anomalies appear in the region where the upward curvature of isentropic surfaces is located. e results shown in Figures 9(d) and 9(h) are consistent with the study from Morcrette et al. [77] that the upward displacement of isentropic surfaces can lead to an upper-level cold pool, which subsequently causes a reduction in static stability beneath the PV anomaly. is, under suitable conditions, will promote deep convection. erefore, the upperlevel PV anomalies and their associated strong instability in the middle troposphere can trigger convective activities at the time = 0 day.

Conclusions
Based on the TRMM and 6-hourly ERA5 and ERA5.1 datasets, this study implements the composite approach to analyze anomalous signals near the tropopause before the OCS onset over the TP. Based on the TRMM data, 41 OCS events over the TP are identified. Using the high-resolution ERA5 and ERA5.1 reanalysis datasets, the tropopause height is stable at the maximum height at the 7th and 5th day before the OCS onset. It then descends significantly from the time = −5th day to −1st day. One day before and on the day of the OCS onset, the tropopause height is obviously decreased, corresponding to the increase of the tropopause temperature. At the time = −5th day, the upward motion in the troposphere is the strongest, corresponding to highest tropopause height. From the time = −1st day to 1st day, there are strong ascending motions at 500-300 hPa but weak descending motions near the tropopause. e change in    Figure 9: e composites of longitude-pressure cross section of (a, b, c, d) temperature anomaly (units: K, color contours) and potential temperature (units: K, black lines, contour interval: 5 K), and (e, f, g, h) static stability anomaly (units: K/hPa) at 34°N for the (a, e) 3rd day, (b, f ) 2nd day, (c, g) 1st day, and (d, h) 0 day before the OCS onset for 41 OCS events. e black dotted areas indicate that the anomalies are statistically significant at a 95% confidence level (based on a two-sided Student's t-test). e red lines show the contours of 1, 2, and 3.5 PV units. tropopause height accompanying OCS is closely related with the evolution of vertical velocity. It is possible that the decreasing of the tropopause height one day before and on the day of OCS onset is beneficial to the occurrence of OCS.
It is proposed that the decreasing of the tropopause height on the day of OCS onset is associated with frequent tropopause fold events over the eastern TP. Analysis of ERA5 and ERA5.1 reanalysis data reveals that the tropopause fold events are caused by a cold trough intrusion from the north and the southeastward movement of upperlevel westerly jet stream. e positive PV anomalies on 350 K isentropic surface at 96°-99°E can be noted in the descending region of the tropopause height at the time = −1st day and 0 day. It is possible that the stratospheric air with higher PV values invades into the troposphere and accumulates as the decreasing of the tropopause height. With the deepening of the tropopause fold, the area behind the fold is accompanied by significant downward motion near the tropopause at around 94°-97.5°E, while the area beneath the fold in the troposphere is marked by prevailing upward motion at 500-300 hPa at 96°-98.5°E on the day of OCS onset. at is, when a strong tropopause fold event occurs, there is not only strong downward transport of air mass from the stratosphere, but also upward motion in the troposphere beneath the folding region. e vertical velocity near the depressed tropopause appears alternately between the positive and negative centers from the time = −3rd day to 0 day, which is related to the baroclinic processes. Furthermore, the upward displacement of isentropic surfaces leads to an upper-level cold pool, which causes a reduction in static stability beneath the PV anomaly on the day of OCS onset. e upper-level PV anomalies and their associated strong instability in the midtroposphere can trigger convective activities by releasing potential instability on the day of the OCS onset. e overshooting convection is more likely to occur due to lower tropopause height, although the upward motion in the troposphere is not the strongest.
Data Availability e ERA5 reanalysis data used to support the findings of this study are available at https://www.ecmwf.int/en/forecasts/ datasets/reanalysis-datasets/era5. e TRMM database is provided by the University of Utah via their website (http:// trmm.chpc.utah.edu/).

Conflicts of Interest
e authors declare that they have no conflicts of interest.