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We counted the frequency distribution of LLJs at different heights (Fig. 4a). LLJs in the Wuhan area occurred more frequently between 300 and 1200 m and were most frequent (30 occurrences) between 900 and 1200 m. The frequency decreased sharply above 1200 m. SLLJs mainly occurred at altitudes of 1800–3300 m, with a maximum of 20 occurrences.
Figure 4. Statistical plots based on intensive sounding observational data show (a) the frequency of LLJs at different altitudes and (b) the wind velocity observational profile for jets (red line) and non-jets (pink line).
Figures 4a and 4b both show that the vertical structure of LLJs during the mei-yu season in the middle reaches of the Yangtze River was mainly characterized by the vertical structure of BLJs, with an average height of about 1200 m and an average intensity >8.5 m s−1. Below 4000 m, the non-jet composite wind speed was significantly lower than that of the jet composite. However, the observed non-jet profile in the Wuhan area also had obvious nose-like features at lower levels.
Du et al. (2012) found that SLLJs in Shanghai occurred more frequently and with more intensity during the mei-yu season. In contrast, BLJs occurred more frequently and with greater intensity in Wuhan during the 2010 mei-yu season, and the observations indicated that they differed significantly from the jets in Shanghai. This unique phenomenon of LLJs in the middle reaches of Yangtze River during the mei-yu season further confirms the need for our study.
The low-level wind speed in Wuhan showed significant diurnal variations, and the diurnal variation of the composite jet wind speed profile was opposite to that of the composite non-jet wind speed profile. When jets were observed, the wind speed above 1000 m was greater during the day than at night. The diurnal variation of the wind speed was relatively complex below 1000 m, but, in general, the intensity of nocturnal jets was slightly greater than that of daytime jets. The composite non-jet profiles showed slightly higher wind speeds at night than during the day, which was most pronounced below 600 m.
Previous studies have shown that the diurnal variation of BLJs becomes insignificant when there are mid-altitude jets above them (Zhang et al., 2007); therefore, we only discuss pure BLJ and pure SLLJ conditions to reveal the diurnal variation of the vertical structure of BLJs more clearly. The diurnal variation of the vertical structure of pure BLJs was the opposite of that of pure SLLJs, with the speed of BLJs greater at night and the speed of SLLJs greater during the day. The BLJs had the highest wind speeds at 0200 LST when the composite wind speed exceeded 14 m s−1. The wind speed began to decrease after 0200 LST. The nose of the BLJ varied in altitude from 600 to 1200 m. The SLLJ was strongest at 1100 LST, with the lowest wind speed occurring at 1700 LST.
The structure of DLLJs was more pronounced at night, with stronger BLJ and SLLJ wind speeds at night and greater vertical shear. The BLJs in the DLLJ were significantly stronger than the SLLJs (Fig. 5). The evolutionary features of the double LLJs at different hours (Figs. 5e-f) show that the DLLJs were strongest at 0200 LST when the BLJ and SLLJ wind speeds reached a maximum. The BLJs were less variable in height, and the nose-like features were always evident. In contrast, SLLJs showed a large variation with height, and the nose-like features of the composite profiles were correspondingly weak and highly variable.
Figure 5. Diurnal variation of the composite observational profile in Wuhan during (a) LLJ observational events, (b) non-LLJ observational events, (c) pure BLJ events, and (d) pure SLLJ events. (e) Diurnal variation of DLLJs and (f) variation in DLLJs at different times in Wuhan. These are statistical plots based on intensive sounding observational data.
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Because the number of observations in Wuhan at 0200 LST was significantly less than that at other hours (about 42 for other hours, but only 32 at 0200 LST), a standard frequency was selected to analyze the daily variation of the jets: Rt = NJETt/Nt × 100, where Rt represents the frequency of jets at hour t, NJETt represents the occurrence frequency of the jets at hour t and Nt represents the total number of observations at hour t.
In conjunction with the diurnal variation of the LLJs (Fig. 6a), the jet-like profile and the occurrence frequency of LLJs in Wuhan showed a double-peak structure during the mei-yu season. There was only a small difference between the primary (0800 LST) and secondary (2300 LST) peaks in the frequency of LLJs. The primary peak of the jet-like profile was recorded at 1100 LST, three hours after the primary peak of the LLJs. Whiteman et al. (1997) reported that the primary and secondary peaks in the frequency of LLJs in Oklahoma during the warm season were at 2300 CST and 0500 CST, respectively. Therefore, the times of the two peaks in the middle reaches of the Yangtze River were roughly consistent with the results of Whiteman et al. (1997), indicating that the patterns of development of LLJs in Oklahoma and Wuhan were similar. However, the primary and secondary peaks of the LLJ frequency in the two regions were diurnally opposite, with the greatest frequency occurring during the day in the middle reaches of the Yangtze River (with the secondary peak at night) and during the night in Oklahoma in the USA (with the secondary peak in the daytime), suggesting that the influence of local factors on LLJs in these regions differs. These differences between the two regions may be due to the specific weather systems in the middle reaches of the Yangtze River during the mei-yu season, such as the mei-yu front, which is mei-yuusually most vigorous in the early morning. The mesoscale circulation caused by the latent heat of condensation of the mei-yu front affects the wind speed of LLJs (Qian et al., 2004), resulting in the unique diurnal variability of LLJs in the middle reaches of the Yangtze River.
Figure 6. (a) Occurrence frequencies of jet-like profiles (gray bars) and jet profiles (red bars; including BLJs and SLLJs) in Wuhan at different times. (b) Daily variation of the frequencies of BLJs (red line) and SLLJs (blue line) in Wuhan; 2000−0500 LST represents nighttime, and 0800- 1700 LST represents daytime. These plots are statistically based on intensive sounding observational data.
Figure 6b shows that BLJs mainly occur at night. The frequency of BLJs showed a double-peak structure, with the maximum at 2300 LST and a second peak at 0800 LST. The frequency of BLJs decreased significantly after 0800 LST. The diurnal variation of SLLJs was the opposite of that of BLJs, occurring mainly during the day and most frequently at 0800 LST. The co-occurrence of the peak frequencies of BLJs and SLLJs at 0800 LST made LLJs, as a whole, most frequent at 0800 LST (Fig. 6a).
An interesting phenomenon in Wuhan is that the frequency of BLJs decreased rapidly after 0800 LST, reached a minimum at 1700 LST, but increased again at night. This may be because the mixed layer started to develop after 0800 LST, causing the turbulent mixing in the boundary layer to intensify, which increased the frictional turbulent drag. The vertical distribution of the wind speed in the boundary layer tended to be uniform, leading to a weakening or even the disappearance of the jets. The frequency of BLJs began to increase again at 2000 LST due to the development of a stable nocturnal boundary layer. The stable nocturnal boundary layer is primarily influenced by surface radiative cooling, with atmospheric temperatures decreasing more rapidly near the surface, resulting in a shallow inversion layer in the lower troposphere. Turbulent mixing is weak at night, and any turbulent friction becomes decoupled when the wind speed in the boundary layer is mainly influenced by surface friction drag. As a result, wind speeds are lower near the surface and stronger at the upper levels, leading to the formation of jets (Blackadar, 1957).
Table 1 shows that the frequency rate of BLJs in Wuhan was slightly higher at night than during the day, but their average height was higher during the day (941.2 m) than at night (875.9 m). The diurnal variation of the mean height of SLLJs was opposite to that of BLJs, with a higher frequency rate during the day but a higher mean height at night (2676.3 m) than during the day (2474.3 m). The mean heights of BLJs and SLLJs in Wuhan were both larger than their corresponding median values and showed a positively skewed distribution. The standard deviation of the height of SLLJs was about twice that of BLJs, indicating a high degree of relative dispersion among the SLLJs.
Frequency rate (%) Height Mean (m) Median (m) Standard deviation (m) Minimum (m) Maximum (m) BLJ Day 27.17 941.2 915 322.6 180 1500 Night 30 875.9 870 312.6 180 1500 SLLJ Day 37.57 2474.3 2370 618.8 1515 3960 Night 31.25 2676.3 2670 557.3 1575 3825 Table 1. Height and frequency rate of BLJs and SLLJs in Wuhan
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The BLJs in the Wuhan area were generally southwesterly, with wind speeds up to 20 m s−1. The frequencies of BLJs in the SSW and WSW directions were 37 and 36, respectively, accounting for 76.84% of the total (n = 95). The frequency of BLJs in the other three quadrants decreased sharply, although the northeasterly direction was a sub-high-frequency region with a significant decrease in wind speed (Fig. 7a). The wind direction of maximum frequency for the SLLJs was still dominated by southwesterly winds, with wind speeds of up to 23 m s−1. However, the wind direction of SLLJs was more westerly than that of the BLJs, and the frequency of northeasterly jets increased significantly (Fig. 7b). The highest frequency wind direction for the SLLJs was from the WSW, followed by westerly winds and then by winds from an NNE direction.
Figure 7. Wind roses summarizing all the wind speeds (units: m s−1) and directions of (a) BLJs and (b) SLJs observed by radiosondes in Wuhan. Composite wind stream and geopotential height (red contours, units: dagpm) at 800 hPa from the ERA5 dataset during (c) southwesterly SLLJs and (d) northeasterly SLLJs. The gray shading represents the topography at 800 hPa. The blue triangle represents the location of Wuhan.
When Vanderwende et al. (2015) studied jets below 2 km in the Iowa region of the USA, they found that the jets were almost non-existent in the first quadrant. In contrast, in the middle reaches of the Yangtze River, the first quadrant had a moderate frequency of jets, indicating that these jets differed from those in the USA. This also confirms the need for this study.
Based on these characteristics, we further analyzed the causes of the formation of southwesterly oriented SLLJs and northeasterly oriented SLLJs. At 800 hPa, the formation of southwesterly oriented SLLJs in the middle reaches of the Yangtze River was closely related to the southwest monsoon. The main system of influence was the low-pressure trough at 800 hPa. Wuhan was in front of this trough and was influenced by southwesterly winds. The weather conditions influencing the northeasterly oriented SLLJs were very different from that of the southwesterly oriented SLLJs. There was an anticyclonic and a cyclonic system to the northwest and southeast of Wuhan, respectively, which means that the Wuhan area was controlled by northeasterly winds.
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We used the ERA5 reanalysis dataset to make a preliminary analysis of the formation mechanism of LLJs in the middle reaches of Yangtze River during the 2010 mei-yu season. First, we verified the validity of the ERA5 reanalysis data for the simulation of LLJs in the Wuhan area during the mei-yu season. In the following developments, the radiosonde sounding data are grouped according to LLJ events and non-LLJ events. We then used the LLJ events chosen from the sounding data to select the ERA5 data at the corresponding time and to plot the mean vertical profile; the same process was used for non-LLJ events.
Figure 8 shows the wind speed and wind direction profiles from the radiosonde sounding data and ERA5 reanalysis dataset from 975 to 400 hPa during the LLJ (Fig. 8a) and non-LLJ (Fig. 8b) events. In terms of the vertical structure, the ERA5 reanalysis data agree fairly well with both LLJ and non-LLJ events in the Wuhan area, where the ERA5 simulation results for the jet core of LLJs are consistent with the sounding observations (Fig. 8a). This shows that the ERA5 reanalysis dataset can effectively simulate the structure of LLJs in Wuhan. Therefore, we used the ERA5 reanalysis dataset to determine the weather conditions favorable for the formation of LLJs during the mei-yu period.
Figure 8. Profiles of the mean vertical wind speed (lines; units: m s-1) and direction (crosses; units: degrees) from the radiosonde sounding observations (red) and the ERA5 dataset (pink) in (a) LLJ and (b) non-LLJ events. The average (c, d) 800- and (e, f) 875-hPa geopotential height (shading; units: dagpm), wind fields (wind barbs; units: m s−1; the black and white wind barbs represent wind speeds greater than and less than 6 m s−1, respectively), equivalent temperature (deep pink contours; units: K) and the 500 hPa geopotential height (cyan contours; units: dagpm) in (c, e) LLJ and (d, f) non-LLJ events during the mei-yu period in 2010. The average (g) daytime and (h) nighttime 875-hPa geopotential height (shading; units: dagpm), wind fields (wind barbs; units: m s−1; the black and white wind barbs represent wind speeds greater than and less than 6 m s−1, respectively), equivalent temperature (deep pink contours; units: K) and the 500-hPa geopotential height (cyan contours; units: dagpm) in LLJ events. The gray shading represents the topography. The red triangle represents the location of Wuhan.
Many scientific studies have been conducted on the formation and development of LLJs. The formation and daily variation of LLJs vary slightly from region to region and are influenced by local diurnal oscillations and weather systems (Blackadar, 1957; Li and Chen, 1998; Lin et al., 2011; Du et al., 2012). Du et al. (2012) showed that the mei-yu front could extend to lower levels during the mei-yu season and affect both SLLJs and BLJs.
We analyzed the formation mechanism of LLJs in the middle reaches of the Yangtze River at 800 hPa and 875 hPa. Figures 8c–f show that the change in the position of the mei-yu front influenced the formation of LLJs in Wuhan. Wuhan was located on the south side of the mei-yu front during LLJ events at both 800 hPa and 875 hPa, whereas it was located on the north side of the mei-yu front in non-LLJ events. The latent heat of condensation on the mei-yu front enhanced the low-level wind field via the mesoscale circulation field (Qian et al., 2004).
The northwest Pacific subtropical high and the low-pressure system over the eastern Tibetan Plateau also significantly affected the formation and development of LLJs in the middle reaches of the Yangtze River. The northwest Pacific subtropical high intensified its westward extension in LLJ events, and the westward ridge point was located at 110°E (115°E in non-LLJ events), which gave the southwesterly airflow from its periphery more influence in the middle reaches of the Yangtze River and favored the formation of LLJs.
The cyclonic circulation near the Sichuan basin was also more pronounced, and the low-pressure system was stronger. Wuhan is located between a strong high-pressure system and a low-pressure system, which causes the pressure gradient to increase in the middle reaches of the Yangtze River, as evidenced by the mid- and low-level geopotential height fields. This large-scale horizontal pressure gradient increased the wind speed in the mid-to-lower levels, promoting the formation and development of LLJs (Xu et al., 2004). Therefore, the influential systems for the formation of LLJs in the middle reaches of the Yangtze River were the mei-yu front, the northwest Pacific subtropical high, and the low-pressure system in the eastern Tibetan Plateau.
We conducted a preliminary analysis of the daily variation mechanism of BLJs, the features of which were more significant in Wuhan. Figures 8g–h show that the intensity of BLJs in the middle reaches of the Yangtze River was significantly stronger at night than during the day and was accompanied by a larger gradient in equivalent temperature. This also implies that the stronger nocturnal mei-yu front promoted the development of the nocturnal BLJs. Regarding geographical location, the BLJs tended to develop stronger when Wuhan was located south of the mei-yu front. The ridge point of the nocturnal northwest Pacific subtropical high was slightly to the west, which was not significantly different from the daytime location (110°E at night, 111°E during the day), but the intensity was significantly stronger at night than during the day. The low-pressure system in the eastern part of the Tibetan Plateau was also stronger at night. Du et al. (2012) identified the inertial oscillation mechanism as the main cause of BLJs in areas with a flat topography.
Frequency rate (%) | Height | ||||||
Mean (m) | Median (m) | Standard deviation (m) | Minimum (m) | Maximum (m) | |||
BLJ | Day | 27.17 | 941.2 | 915 | 322.6 | 180 | 1500 |
Night | 30 | 875.9 | 870 | 312.6 | 180 | 1500 | |
SLLJ | Day | 37.57 | 2474.3 | 2370 | 618.8 | 1515 | 3960 |
Night | 31.25 | 2676.3 | 2670 | 557.3 | 1575 | 3825 |