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According to the literature, the extremely warm SST in the tropical Indian Ocean (Wang et al., 2021a) induced a westwardly extended anticyclone of unprecedented strength in the subtropical western Pacific (Clark et al., 2021) relative to climatology. The vital water vapor transport by the anomalous anticyclone, associated with the anomalous ascending motions induced by the enhanced southwesterly jet, caused heavy and persistent rainfall over East China during the summer of 2020 (Niu et al., 2021; Wang et al., 2021b).
Figure 2 shows the environmental background in May, June, and July from the ERA-5 reanalysis. The location of the summer monsoon rainband is primarily determined by the western Pacific subtropical high (WPSH, Ding and Chan, 2005). Specifically, after the onset of the EASM in May 2020, a monsoonal rainband was positioned over South/Southeast China to South Japan (Figs. 2a–c). The resulting rainfall center was located over Guangdong, north FJ, and Taiwan (Fig. 2d). The WPSH then jumps northward in early June (two weeks earlier than the climatology, Ding et al., 2021). Its ridgeline lies north of 20°N after the jump (Fig. 2e). During this period, South China and FJ were controlled by the WPSH, and the relative humidity and vorticity in FJ were much lower; consequently, there were fewer rainy days than usual.
Figure 2. Monthly mean horizontal wind (wind arrows, m s–1), geopotential height (contour, hPa), and (a, e, i) 500-hPa absolute vorticity (shading, 10–5 s–1), (b, f, j) 700-hPa relative humidity (shading, %), and (c, g, k) 850-hPa temperature (shading, °C) from the ERA-5 reanalysis in (top) May, (middle) June, and (bottom) July. The distribution of the monthly rainfall amount (mm) in (d) May, (h) June, and (l) July.
In contrast, the strengthened southwesterly flow carried abundant moisture from the ocean to the YHRV and converged with cold air from Northeast Asia (Figs. 2f, g, j, k). Subsequently, the slowly northward-moving rainband was subjected to increased convective instability and the early onset of the heaviest and most persistent mei-yu rainfall over the YHRV (Figs. 2h, l). Owing to the earlier northward migration, the rainfall in FJ and JS was approximately –50% and +(50%−150%) that of climatology, respectively (Niu et al., 2021; Zhou et al., 2021).
The disdrometer observed relative rainfall contributions from convective versus the total rainfall amount at each site is shown in Fig. 3a. Considering the expected variations at each site, the Parsivel-observed convective rainfall contribution was comparable between JS (47.89%) and FJ (45.47%). The observed maximum rainfall amount during the mei-yu season in JS was 707.33 mm, whereas that during the pre-summer season in FJ was 312.36 mm. On average, stations in JS experienced rainfall that was nearly twice as heavy than in FJ, with respective depths of 439.64 mm and 225.65 mm. The mean convective daily rainfall amount for FJ and JS was 2.52 and 5.13 mm d–1, with the daily number count of 1-min samples being 120.51% higher in JS (Fig. 3b). The respective daily amounts of stratiform rain were 2.89 and 5.34 mm d–1, and there were 62.62% more samples in JS (Fig. 3c). Generally, the duration of pre-summer rainfall in FJ is significantly lower than usual, while the mei-yu rainfall in JS showed the opposite effect.
Figure 3. (a) Rainfall contribution of convective versus total rainfall amount from disdrometer observations, and the rainfall amount versus number counts of raining minutes per day for (b) convective and (c) stratiform rain in FJ (blue dots) and JS (red dots). Error bars represent the standard deviation of the averaged values.
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The spatial distributions of the averaged Dm and Nt from each site in FJ and JS are shown in Fig. 4. The vast majority of the averaged convective Nt for pre-summer rainfall in FJ was concentrated around 1000 to 1600 m–3, with 3 out of 30 sites being between 800–1000 m–3. The convective Nt of the mei-yu rainfall in JS was approximately 800–1200 m–3, with 5/66 sites between 600–800 m–3. Despite the regional variability, the pre-summer rainfall is generally characterized by a slightly higher Nt (~200 m–3) than the mei-yu rainfall for both convective and stratiform rain, while the differences in Dm are negligible. In both FJ and JS, the distance between two random observational sites ranges from several kilometers to over 500 km. Considering the wide range of observations, the variability of Dm and Nt within (and between) the pre-summer and mei-yu seasons was small. The results from the dense network of DSD observations over such a wide range may imply near-homogeneous microphysical characteristics during the two periods in the two study areas.
Figure 4. Averaged convective and stratiform Dm (dot sizes) and Nt (colors) at each site in (a, b) FJ and (c, d) JS.
The distribution of the averaged Dm–lgNw pairs at each site also showed inherent similarities between the pre-summer and mei-yu rainfall (Fig. 5). The stratiform Dm–lgNw pairs from FJ and JS showed substantial negative correlation coefficients (CC=–0.89 and –0.77), nearly overlapping with each other. The fitted Dm–lgNw linear relationships using the least-squares method had similar slopes (–1.71 and –1.75), and the same intercept value (5.56), with the coefficient of determination (R2) higher than 0.6 and the root mean square error (RMSE) lower than 0.09. As suggested by Bringi et al. (2003), the reverse distribution of the Dm–lgNw line reflects the different microphysical processes of stratiform rain, ranging from the melting of tiny graupel or smaller rimed ice particles to the melting of large dry snowflakes. The fitted stratiform lines lie to the left of the “stratiform line” in Bringi et al. (2003) with similar negative slopes. This suggests that stratiform rain during the EASM in East China remained steady while moving northward from FJ to JS, with a smaller raindrop diameter than that of the other climatic regimes.
Figure 5. Scatterplot of averaged Dm–lgNw pairs from each site. The blue and cyan squares represent convective and stratiform rain in FJ, and the red- and black-filled circles represent convective and stratiform rain in JS, respectively. The gray rectangles and the pink dashed line correspond to the maritime and continental convective cluster and stratiform line in Bringi et al. (2003). The pink and green symbols represent the averaged convective and stratiform values from the literature. The fitted convective and stratiform lines and relations for convective and stratiform rain for FJ and JS are provided with the corresponding colors. The shading represents the 95% confidence interval of the fitting. CC = correlation coefficient; R2 = coefficient of determination; RMSE = root mean square error.
The convective Dm–lgNw pairs were located around the lower right of the “maritime cluster” in Bringi et al. (2003), implying the near-maritime nature of convective rain in East China. Remarkably, straight convective Dm–lgNw lines were also fitted, as the pairs exhibited a stronger correlation (CC=–0.93 and –0.91) than stratiform rain. The pre-summer line was located to the northeast of the mei-yu line because of the slightly higher concentration of raindrops in FJ. Meanwhile, R2 was higher, whereas the RMSE was smaller for the fitted convective lines, suggesting a stronger negative correlation between Dm and lgNw in convective rain for both FJ and JS.
It is worth noting that although a different rain type classification method was applied in this study, the Dm–lgNw distribution obtained here showed only minor differences compared to that when using the Bringi et al. (2003) scheme. Therefore, the comparative results were general and acceptable. Moreover, based on the distribution of Dm–lgNw pairs using multisource observations from one or a few stations in the same/surrounding climatic regimes, previous DSD studies usually announce the finding of a different characteristic compared with the others. However, such findings are inconclusive because many factors contribute to these “differences”. One of the main reasons for this is the lack of spatial representativeness, with insufficient data samples from one or a few stations.
Using observations from the dense disdrometer network, the features of the statistical EASM rainfall Dm–lgNw pairs recognized here demonstrate that the “differences” in the literature are mainly within the deviations between each site. For example, for convective rain, the summer rainfall in Guangdong, South China (Huo et al., 2019, right triangle), mei-yu rainfall in Hubei, Central China (Fu et al., 2020, plus), and summer/mei-yu rainfall in Taiwan (Chen, 2009, diamond), and Jiangsu (Chen et al., 2013, pentagram; Wen et al., 2017b, down triangle), East China, are all plotted around the derived convective lines. Their averaged stratiform Dm–lgNw pairs are less diverse and lie between the stratiform lines of Bringi et al. (2003) and the newly derived ones.
The large dataset of 96 OTTs observations in this study aids us in the effort of determining whether there is some commonality besides the spatial (FJ and JS) and temporal (pre-summer and mei-yu rainfall) diversity of EASM rainfall microphysics. In this case, the results implied that the “differences” obtained in previous studies should be largely recognized as a deviation in DSD at a specific site and can be well represented by the general characteristics of EASM rainfall microphysics. The similarity in the derived Dm–lgNw lines can be considered a valid and reasonable indicator.
Generally, the overlap of averaged Dm–lgNw pairs from 30 sites in FJ and 66 sites in JS (with similar coefficients of linear fitting), as well as the similarities with the results in the literature, suggest near-homogeneous microphysical characteristics during the northward migration of summer monsoon rainfall, typically from the pre-summer rainfall in South/Southeast China to mei-yu rainfall in the YHRV.
The distributions and statistics of various DSD parameters for the pre-summer and mei-yu rainfall were further compared with the average value and standard deviation in each panel (Fig. 6). Both convective and stratiform rain showed similar distribution patterns for the bulk DSD parameters between the pre-summer and mei-yu rainfall. While most convective and stratiform Dm values range from 1 to 3 mm and 0.5 to 2 mm, respectively, and their distributions all have negative skewness. In contrast, the skewness of convective lgNw (and lgNt) is positive, with a much narrower range than its stratiform counterpart. This suggests large numbers of smaller raindrops in intense rainfall. Because of the slightly higher concentration of raindrops, the corresponding convective Z, R, and LWC values during pre-summer rainfall were slightly larger than those during mei-yu rainfall. The distributions of μ and Λ also exhibited consistent characteristics between these two periods/areas. The only noticeable difference was the higher average Ct value for pre-summer rain in FJ. This phenomenon may have resulted from the higher environmental moisture content in FJ, which is much closer to the South China Sea (the primary water vapor source). Overall, the difference in the DSD parameters (except Ct) between the pre-summer and mei-yu rainfall was minor and smaller than the standard deviation within each period/area.
Figure 6. Histograms of DSD variables and spectra for convective and stratiform rain in FJ and JS. (a–i) Red and black curves: convective and stratiform rain in JS; blue and cyan bars: convective and stratiform rain in FJ, respectively. The averaged value and its standard deviation are given in each panel with the corresponding color.
For comparison, the derived integral rain parameters for convective and stratiform rain during 2020, as well as those from Wen et al. (2017b) for the 2014–15 mei-yu rainfall in Nanjing, Jiangsu province, and Hu et al. (2022b) for the 2019 monsoon rainfall in Xiamen, Fujian province are presented in Table 1. For convective rain, the difference in Dm is within ±0.1 mm, while lgNw (and Nt) have the highest values in Hu et al. (2022b). The slightly higher raindrop concentrations (and the resulting higher R and LWC) in FJ than in JS from the literature are consistent with the present work. For stratiform rain, the differences are considerable but still within the standard deviation of each DSD parameter. These results imply that observations from one or a few stations are not necessarily statistically conclusive to address a “different” characteristic and that regional variability should be reasonably considered to reach a general conclusion.
Rain type Studies Years Dm lgNw Nt R LWC Convective JS 2020 1.80 3.89 871 22.64 1.05 Wen et al. (2017b) 2014−15 1.73 3.84 846 19.10 0.88 FJ 2020 1.84 3.95 1047 24.53 1.29 Hu et al. (2022b) 2019 1.74 4.07 − 23.38 1.21 Stratiform JS 2020 1.06 3.69 200 1.72 0.11 Wen et al. (2017b) 2014−15 1.19 3.67 271 2.16 0.13 FJ 2020 1.00 3.86 269 1.51 0.12 Hu et al. (2022b) 2019 1.24 3.97 − 2.20 0.15 Table 1. Integral rain parameters as derived from the composite raindrop spectra of convective and stratiform rain in FJ and JS and previous studies in each region.
For comparison, the composite spectra of different rain types, R classes, and Z classes also exhibited substantial similarities between the pre-summer and mei-yu rainfall (Fig. 7). All the spectra have peak concentrations mostly in the diameter range of ~0.5 mm with a sharp drop-off towards smaller sizes. It is a typical Parsivel-observed size spectrum at the small end (Tokay et al., 2013; Wen et al., 2016). The role of instrument limitations on missed small-sized drops, and thereby the concave downward shape, has been explained by Wen et al. (2017b) and is not discussed further. Overall, convective rain has a higher concentration in every size bin and a larger maximum diameter than stratiform rain. The stratiform spectra were narrower, with a maximum diameter of approximately 4.7 mm. The raindrop concentration and maximum diameter also increased with increasing R (Fig. 7b), regarding incremental rain rate classes from <5 mm h–1 to 5–10 mm h–1, 10–30 mm h–1 , and >30 mm h–1. Similar characteristics were also observed for the Z classes (Fig. 7c).
Figure 7. Composite raindrop spectrum curves for different (a) rain types, (b) R classes, and (c) Z classes. The solid and dashed lines represent rainfall in JS and FJ, respectively. (d–f) Differences in N(d) between FJ and JS with variable colors corresponding to different classes.
The differences in raindrop concentration between pre-summer and mei-yu rainfall were compared in each size bin by subtracting N(d) of JS from N(d) of FJ (Figs. 7d–f). One can conclude that pre-summer rainfall contains more small drops peaking at ~0.5 mm and extends to 1–2 mm size bins with intense rainfall. Accordingly, the higher Ct (up to 683.89) due to the extra small drops in pre-summer rainfall should be responsible for the slightly higher values of some DSD parameters than mei-yu. The influencing magnitude decreased with an increase in the DSD moment. The lower-ordered parameters (such as Nt) have a more pronounced impact than the higher-ordered ones (such as Z).
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Eight-year GPM-DPR observations were applied to confirm the near-homogeneous DSD characteristics on the ground as derived above and to further investigate the statistics associated with vertical structures of monsoon rainfall microphysics. The Ze, Dm, and lgNw contoured frequencies by altitude diagrams (CFADs) from during April-May-June in FJ and June-July-August in JS are presented in Fig. 8. Note that the contaminated near-surface-level data due to ground clutter (<1 km height) were eliminated from the discussion. Similarities in the statistical vertical structure and evolution of precipitation in these two regions/periods can also be found in the satellite observations, consistent with the rainfall microphysics similarities described in the previous paragraphs from ground-based Parsivel observations.
Figure 8. Vertical profiles of (left) Ze, (middle) Dm, and (right) lgNw for convective (C_) and stratiform (S_) rain in FJ and JS. Shaded colors represent the frequency of occurrence relative to the maximum absolute frequency in the data sample represented in the CFAD. (m–o) The blue and red (black and cyan) lines represent the averaged convective (stratiform) rainfall values in FJ and JS, respectively.
For convective rain of pre-summer rainfall in FJ and mei-yu rainfall in JS, the altitude of the majority (>30% of the maximum frequency) of 30-dBZ distributions for convective rain is near 6-km height, suggesting the general formation of moderate convection within warm clouds (Chen et al., 2019; Wen et al., 2020). The sharp decrease in convective Ze at altitudes above the freezing level indicates a limited amount of large frozen hydrometeors and super-cooled water (Carr et al., 2017; Wen et al., 2020). Consequently, large raindrops were rare near the ground. Below the 0°C isotherm level, the convective Ze continued to increase until a height of 1 km, with the convective core centered at ~32–35 dBZ. The average convective Ze in FJ was only ~1 dBZ higher than in JS.
The corresponding convective Dm and lgNw CFADs exhibited negligible differences. Typically, below the 0°C isotherm level, the average profiles of convective Dm and lgNw for FJ and JS were nearly identical (Figs. 8n, o). From a height of 4 km to ~2 km, the rapid increase in Ze was associated with an increase in both Dm and lgNw, implying the combined effects of coalescence and warm rain accretion, noting that the warm rain microphysical processes related to DSD include rain evaporation, accretion, and sedimentation (Carey and Rutledge, 2000; Zhang et al., 2008). While the coalescence process increased the raindrop size and decreased the concentration, the accretion process had the opposite effect. The evaporation distinctly decreases the concentration of raindrops but should be negligible under such a humid environment in the persistent EASM rainband (Wen et al., 2020). Meanwhile, the DSD often narrows because of size sorting by the differential sedimentation of falling particles (Milbrandt and Yau, 2005; Dawson et al., 2010). However, in a statistical sense, size sorting is transient and does not substantially impact the overall DSD characteristics (Bailey and Hallett, 2009), especially during moderate convection within the widespread stratiform area of quasi-stationary and continuous monsoonal rainfall (Kumjian and Ryzhkov, 2012; Wen et al., 2020). From a height of 2 km downward to 1 km, the convective Dm decreases slightly while the lgNw value continues to increase. These characteristics may have been associated with an overpowered breakup rather than a coalescence process.
For stratiform rain, the CFADs and mean vertical profiles of the examined parameters show an even more homogeneous pattern for FJ and JS. The stratiform Ze and Dm at all altitudes were lower than those of convective rain, with an enhanced reflectivity area (bright band, ~25.5 dBZ) around the 5-km height (near the 0°C isotherm level). The stratiform Ze also decreases rapidly at an altitude above the 0°C isotherm level. In contrast, it shows only a weak decreasing trend (ranging between 20 dBZ and 30 dBZ) when descending toward the ground. The decrease in stratiform Dm and increase in lgNw below the melting layer can be attributed to the breakup process (Rosenfeld and Ulbrich, 2003).
To investigate the potential anomalous characteristics that might be responsible for the heavy rainfall during 2020, the differences in the vertical profiles for convective and stratiform rain in FJ and JS between 2020 and the eight-year statistics were presented in Fig. 9. As shown, monsoon rainfall in 2020 exhibited minor anomalies in the vertical structure of its precipitation microphysics. Typically, convective rain in FJ was slightly weaker, with the maximum difference in Ze being lower than 1 dBZ. In contrast, convective JS rainfall was stronger in 2020 than the eight-year average, but the differences are still lower than 1.5 dBZ (below 14 km height). The convective Dm showed a differential pattern similar to that of Ze, whereas the lgNw did the opposite. In other words, the heavy rainfall during 2020 in JS (FJ) was associated with a slightly stronger (lower) than average convection with a ~0.1 mm larger Dm (~0.1 mm–1 m–3 lower lgNw). The differences in stratiform Ze were still lower than 1 dBZ for both JS and FJ, and they all contain a ~0.8 dBZ stronger bright band. The differences in stratiform Dm and lgNw were even smaller. The comparison of the vertical structure of precipitation between 2020 and the eight-year average revealed a negligible difference in annual EASM rainfall microphysics.
Figure 9. Differences in the vertical profiles of averaged (left) Ze, (middle) Dm, and (right) lgNw for convective (C_) and stratiform (S_) rain in FJ and JS between 2020 and the eight-year statistics.
Generally, the GPM-derived precipitation microphysics is a typical monsoon rainfall feature in East China, which is consistent with polarimetric radar observations (Shusse et al., 2009; Oue et al., 2011, 2015; Chang et al., 2015; Wen et al., 2020; Chen et al., 2022). Both Wen et al. (2020) and the current study target the vital role of warm rain processes during the evolution of the summer/mei-yu convective rainfall in this specific region. It is worth noting that the different working principles, data samples, and processing procedures can all contribute to the differences between the GPM and ground-based observations. Despite their slight differences, the high uniformity of the vertical distribution and pattern of precipitation microphysics between FJ and JS as derived from the GPM (for both summer 2020 and the eight-year average) is another indicator that supports the disdrometer-observed, near-homogeneous DSDs.
In summary, observations from the disdrometer, polarimetric radar, and satellite-borne radar in the present and previous studies cooperatively brought us to a consensus. There was inherent homogeneous precipitation microphysics (with slight regional deviations) during the northward migration of the quasi-stationary EASM front and the associated rainband in East China. With near-homogeneous precipitation microphysics, the long-lasting duration of rainfall, as opposed to differences in precipitation microphysics, was responsible for the record-breaking monsoonal rainfall in 2020 over this specific region.
Rain type | Studies | Years | Dm | lgNw | Nt | R | LWC |
Convective | JS | 2020 | 1.80 | 3.89 | 871 | 22.64 | 1.05 |
Wen et al. (2017b) | 2014−15 | 1.73 | 3.84 | 846 | 19.10 | 0.88 | |
FJ | 2020 | 1.84 | 3.95 | 1047 | 24.53 | 1.29 | |
Hu et al. (2022b) | 2019 | 1.74 | 4.07 | − | 23.38 | 1.21 | |
Stratiform | JS | 2020 | 1.06 | 3.69 | 200 | 1.72 | 0.11 |
Wen et al. (2017b) | 2014−15 | 1.19 | 3.67 | 271 | 2.16 | 0.13 | |
FJ | 2020 | 1.00 | 3.86 | 269 | 1.51 | 0.12 | |
Hu et al. (2022b) | 2019 | 1.24 | 3.97 | − | 2.20 | 0.15 |