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Article

Study on the Boundary Layer of the Haze at Xianyang Airport Based on Multi-Source Detection Data

1
School of Electrical & Electronic Engineering, Shandong University of Technology, Zibo 255000, China
2
Institute of Desert Meteorology, China Meteorological Administration, Urumqi 830002, China
3
The Northwest Regional Air Traffic Administration Bureau, CAAC (Civil Aviation Administration of China), Xi’an 710082, China
4
Department of Mathematics and Computer Science, Royal Military College of Canada, Kingston, ON K7K 7B4, Canada
*
Author to whom correspondence should be addressed.
Remote Sens. 2023, 15(3), 641; https://doi.org/10.3390/rs15030641
Submission received: 19 November 2022 / Revised: 19 January 2023 / Accepted: 19 January 2023 / Published: 21 January 2023

Abstract

:
To reveal the high-resolution atmospheric and statistical characteristics of haze events within the boundary layer (BL) in different months, this study conducted a combined detection experiment using a wind-profiling radar, a microwave radiometer, and an ambient particulate monitor on 1230 haze events occurring at Xianyang Airport from 2016 to 2021. First, the boundary layer heights (BLHs) of the haze events were calculated using the atmospheric refractive index structure constant, wind direction and speed, and these were verified against reanalysis data from ERA-Interim. Spatial–temporal evolution and statistical characteristics of temperature, and relative humidity and horizontal wind during haze events, were then analyzed. Finally, the relationships between the BLH and AQI (air quality index) and PM 2.5 during the haze events were analyzed. The results indicate that the average BLHs during haze events at Xianyang Airport were generally lower than 1000 m. Moreover, the average BLHs in December and January were distributed in the range of 200–600 m, and lower than that in June and July, in a range of 500–1100 m. Furthermore, the maximum value of the average BLH appears at 13:00–15:00. When the temperature was low in the morning, the stratification difference was small and the sensible heat flux between ground and air was still weak, leading to a low BLH value. Meanwhile, when the air quality was poor, the relative humidity was relatively large, and the corresponding AQI and PM 2.5 were very large. Subsequently, when the temperature gradually increased with time, the heat flux and the average BLH also gradually increased. Moreover, the relative humidity within the BL decreased, and the corresponding AQI and PM 2.5 also gradually decreased, with the corresponding air quality improving accordingly. The results obtained herein provide a key reference for the preparedness of haze events.

Graphical Abstract

1. Introduction

In meteorology, haze is an atmospheric condition attributed to ambient fine particulates in the lower atmosphere; moreover, these particulates can be suspended for prolonged periods and induce air pollution [1,2,3]. Despite the recent reduction in air pollutants and their precursors, haze events still occur frequently, and air pollution levels are still substantially high in China [4,5,6,7]. Haze exerts notable effects on visibility, radiation budget, and even climate change [8,9,10,11]; moreover, poor air quality caused by haze can be a threat to human health, in the form of various respiratory and cardiovascular diseases which cause over 3 million premature deaths every year globally [12,13]. Therefore, reducing haze events and improving air quality are still important measures for the health of people living in China [14].
Based on previous studies, haze results from the combined effects of the accumulation of a high number of aerosol particles and adverse meteorological conditions [15,16,17,18]. Meanwhile, the meteorological conditions of haze episodes are often proposed to be interlinked with the boundary layer (BL). Moreover, the BL is an essential element for understanding the vertical transfer of momentum, energy, and the mining of pollutants in the lower layer of the atmosphere [19,20,21]. Many previous researchers investigated correlations between BL meteorological conditions and high-pollution events, and they found that persistent and explosive haze events are commonly associated with mechanisms such as weak winds from weak pressure systems, high humidity, and a relatively stable BL. However, rapid disappearance of air pollution is commonly due to strong winds with a surface high pressure within the mining layer [22,23,24]. Moreover, decreasing surface temperature and rising humidity can increase air pollution, and suppress the development of the BL [25,26]. Furthermore, the mining layer height, which relates to solar radiation, exerts a strong influence on the development of haze events [27,28,29]. Most previous studies focused on the formation and dramatic development of a single severe haze event, with few detailed studies investigating the high-resolution atmospheric and statistical characteristics of the haze events within the BL in different months due to a lack of meteorological and aerosol observations.
Haze is a frequent weather condition at Xianyang Airport, which is the biggest airport in Northwest China. It not only seriously reduces the air quality, but also disturbs traffic. To reveal the spatial–temporal variation in meteorological characteristics and air quality during haze events within the BL, a wind-profiling radar, microwave radiometer, and ambient particulate monitor, were combined to detect the haze events occurring at Xianyang Airport. Air temperature and relative humidity can be observed using a microwave radiometer; when these were compared to air sounding profiles, there was a good correlation [30,31,32,33,34]. Furthermore, the direction and speed of horizontal winds can be detected using a wind-profiling radar in real time. Compared with meteorological radiosondes, which only can acquire atmospheric factors at 08:00 BT and 20:00 BT [35] (BT stands for Beijing time), high-resolution observations using a wind-profiling radar and microwave radiometer are more effective for analyzing the characteristics of haze events.
The sections in this paper are as follows. Section 2 introduces the detection equipment and data. Section 3 describes the method for the boundary layer height (BLH) using the atmospheric refractive index structure constant ( C n 2 ), and the wind directions and speeds detected by the wind-profiling radar. Section 4 analyzes the spatial–temporal and statistical variation characteristics of the meteorological factors within the boundary layers during haze events in different months. Section 5 analyzes the variation characteristics of PM 2.5 (particulate matter with a diameter < 2.5 μm), PM 10 (particulate matter with a diameter < 10 μm) and AQI (air quality index) within the boundary layers during haze events in different months.

2. Materials and Methods

2.1. Equipment and Data

The main instruments used in this study were a wind-profiling radar (CFL), microwave radiometer and an ambient particulate monitor. The CFL-03 wind-profiling radar (shown in Figure 1b) is a boundary layer wind-profiling radar, developed by the 23rd Research Institute of China Aerospace Science and Industry Corporation (the parameters are shown in Table 1). This radar operates stably and can monitor the C n 2 , and horizontal wind speeds and wind directions in real time. The microwave radiometer (shown in Figure 1c) was developed by the China Ordnance 206 Institute; it comprises 21 water vapor channels with a frequency range of 22–30 GHz, 14 temperature channels with a frequency range of 51–59 GHz and 1 infrared channel, which can detect the temperature and relative humidity of the vertical height in real time. The ambient particulate monitor can monitor data such as PM 2.5 and PM 10 in the atmosphere per hour.
In this study, the detection site was located at Xianyang Airport (point A in Figure 1a), which is surrounded by mountains, and where haze frequently occurs. According to the China Civil Aviation Ground Observation Rules, haze exists when visibility is <7 km and there is low-level relative humidity of <75%. Based on visibility detected by the visibility meter and relative humidity observed by the weather observation instrument, the trained observers recorded 1230 haze events occurred from 2016 to 2021. The specific number of occurrences per month is shown in Table 2, of which the occurrence frequency in December, January and February is relatively high (all more than 150 times), while the occurrence frequency in May, June and July is less (all below 60 times); the time at which the haze events occurred was concentrated between 06:00 BT and 18:00 BT. Moreover, 60 no-haze events (5 per month) from 2020 to 2021 were also analyzed; visibility was >10 km and the record by trained observers was sunny without any other weather conditions.
This study analyzed the L structure of haze events occurring at Xianyang Airport between 08:00 and 18:00 (BT), in the period 2016 to 2021, using the C n 2 , horizontal wind, temperature, RH, PM 2.5 , PM 10 and AQI, jointly detected by the wind-profiling radar, the microwave radiometer and the ambient particulate monitor.

2.2. The Method of Determining the BLH

The BL is a thin layer where the energy and dynamics of the atmosphere interact with the ground; the convective motion of the atmosphere within the BL is significantly greater than that above the BL [36,37]. Due to the relatively stable operation of the CFL, it can effectively detect the high–resolution C n 2 , and horizontal wind speeds and wind directions in real time. As the C n 2 detected by the CFL can be expressed as Equation (1) using the temperature structure constant C T 2 , the humidity structure constant C e 2 and the temperature and humidity structure change constant C T e 2 , the C n 2 can effectively reflect the vertical variation characteristics of atmospheric temperature and humidity. Furthermore, the C n 2 is used to determine the BLH, based on the characteristic that the vertical gradient of temperature and humidity within the BL is greater than that above the BL (e.g., Liu et al. [38], Pichugina et al. [39]).
C n 2 = a 2 C T 2 + b 2 C e 2 2 a b C T e 2
As the horizontal wind speed and direction within the BL are significantly different from those above the BL, many previous studies (e.g., Pichugina et al. [40], Vickers et al. [41]) also used the vertical variation characteristics of the horizontal wind speed and wind direction to effectively inverse the BLH.
Based on the previous studies, this paper used the C n 2 , and horizontal wind speed and direction detected by the CFL to determine the BLH. The main steps were as follows:
First, the gradient changes ( Δ C ) of the atmospheric refractive index structure constants between the adjacent vertical bins were calculated, and then the maximum Δ C m a x in the vertical height was found. Subsequent to this, the Δ C at every bin was normalized by dividing Δ C m a x to obtain the normal gradient change ( Δ C a ). The equations are expressed as Equation (2), in which C i + 1 2 and C i 2 are the atmospheric refractive index structure constants of the two adjacent vertical bins, respectively.
{ Δ C = C i + 1 2 C i 2 Δ C a = Δ C / Δ C m a x
Second, according to the method used by Liu et al. [38], the wind directions and wind speeds of the three adjacent vertical bins were used to calculate the variances of wind direction and wind speed (respectively expressed as SD and SS), following which the maximum variances of the wind direction and wind speed in the vertical height (respectively expressed as S D m a x and S S m a x ) were found. Subsequent to this, the SD (SS) were normalized by dividing S D m a x ( S S m a x ) to obtain the normal variances of wind direction and wind speed (respectively expressed as S D a and S S a ). The equation is expressed as Equation (3).
{ S D a = S D / S D m a x S S a = S S / S S m a x
Finally, as the BLHs at Xianyang Airport were less than 3000 m, Δ C a , S D a and S S a at the same height (less than 3000 m) were used to obtain the judgment value HC. The equation is expressed as Equation (4). Moreover, the HCs of different heights were compared to determine the maximum H C m a x . The height corresponding to H C m a x was subsequently determined as the BLH.
H C = Δ C a × α   +   0.5 ( S D a + S S a ) × ( 1 α )
In Equation (4), α is an adjust parameter. Depending on whether the low-atmospheric layer is well-mixed or not, α can be expressed as Equation (5), in which T expresses Beijing time and m is the detection times per hour of the CFL (m = 12 in this study). When the low-atmospheric layer is not well-mixed, the α is less than 1 and the BLH is mainly determined by the wind shear around the BLH, especially in the morning (8:00–9:00 BT). However, the α is equal to 1 and the BLH is determined by the turbulence of the temperature and RH, when the atmospheric layer is well-mixed (13:00–15:00 BT).
α = {   ( T 8 ) · m 60   8 T < 13 1   13 T 15 ( T 15 ) · m 36   15 T 18
To verify the reliability of this algorithm, two haze events from 8:00 to 18:00 on 4 November 2016 and from 8:00 to 18:00 on 4 March 2021, and one no-haze event from 8:00 to 18:00 on 3 November 2021 were selected to judge the BLHs (black line in Figure 2). Furthermore, compared with the BLHs of the time from 12:00 to 16:00 (black circles in Figure 2 are the reanalysis data from ERA-Interim https://cds.climate.copernicus.eu/cdsapp#!/dataset/reanalysis-era5-single-levels?tab=form), the two data points were consistent, with the difference being less than 100 m, which indicates that the BLH inversion by this algorithm is credible. A more in-depth discussion of this method is found in the Discussion section.

3. Results

3.1. Spatial-Temporal Characteristics of Typical Haze Events within the BL in Different Months

In order to examine the evolution characteristics of the boundary layer structure during the haze events at Xianyang Airport, the haze events occurring on 31 January 2020, 10 February 2020, 4 March 2021, 4 April 2020, 3 May 2021, 11 June 2020, 13 July 2020, 3 August 2020, 25 September 2020, 25 October 2020, 4 November 2016, and 23 December 2016, were selected as typical cases for different months. Their corresponding data were used in the analysis of the spatial–temporal evolution characteristics of temperature, relative humidity, and wind.

3.1.1. Spatial–Temporal Characteristics of Temperature and Horizontal Wind within the BL during Typical Haze Events

The spatial–temporal evolution of the temperature and horizontal wind within the BL in the typical haze process at Xianyang Airport were obtained using temperature and wind data detected by the microwave radiometer or the CFL. As shown in Figure 3 (the blue lines are the BLHs with time), at the start of sunrise (8:00–9:00), the ground temperature was very low, and the low altitude was a stable boundary layer with a low BLH (less than 500 m). Furthermore, with the increase in solar radiation (9:00–12:00), the ground temperature gradually increased, and the BLH also increased gradually. Subsequently, when time reached noon (13:00–15:00), the temperature reached its maximum value, with the BLH also reaching its maximum. However, as the solar radiation began to weaken after noon (16:00–17:00), the temperature began to fall and the BLH gradually decreased. When the sun began to set (18:00), the temperature fell significantly, with the BLH falling to 500 m again.
Comparing July with the highest temperature (Figure 3g) and January with the lowest temperature (Figure 3a), it is seen that the ground heated more rapidly with time than it did in January due to the greater intensity of solar radiation in July. During July, the BLH also rose more rapidly and its maximum value reached 1300 m at 14:00. However, during January, the solar radiation intensity was weaker, with the ground temperature increasing slowly; moreover, the corresponding BLH rose slowly and its maximum value was just over 500 m. One explanation is that the higher July temperatures and stronger solar radiation resulted in the sensible heat flux being larger and the effect of turbulence and mining being stronger. Correspondingly, the BLH increased more rapidly and was higher.
As shown in Figure 3, generally, the wind direction within the BL was northeasterly or northwesterly, and the wind speed was lower than 5 m/s. There was also wind shear (changes in wind direction and speed) at the top of the BL. Moreover, the wind speed did not vary much with time, but the wind direction changed significantly from 12:00 to 15:00, which indicates that there was a certain turbulent motion within the BL during this period. Furthermore, this turbulent motion could have accelerated the exchange of heat and the mining of water vapor in the atmosphere, thereby promoting the elevation of BLH. Additionally, when the BLH increased, the turbulent motion within the BL may also have accelerated the mixing of pollutant particles. This probably led to dilution of the concentration of pollutants and reductions in PM 2.5 and PM 10 from 12:00 to 15:00.
Overall, the temperature within the BL was significantly higher than that above the BL during the haze events at Xianyang Airport. Moreover, the change in BLH with time positively correlated with temperature. When the temperature increased with time, the BLH also increased; however, when the temperature decreased with time, the BLH also decreased. In addition, the higher temperature and the stronger the solar radiation, the more rapidly and higher the BLH grows. The wind speed within the BL was relatively small (basically lower than 5 m/s) and its variation with time was small during the haze events, which was conducive to the accumulation of pollutants and easy development of haze. In addition, there was some wind shear at the top of the BL.

3.1.2. Spatial—Temporal Characteristics of Relative Humidity within the BL during Typical Haze Events

Figure 4 illustrates the spatial–temporal evolution of the relative humidity within the BL of the typical haze process at Xianyang Airport (where the black line is the variety of the BLH with time). Comparing Figure 3 and Figure 4, the characteristics of relative humidity and temperature with time are in opposition. As shown for the period October–December (Figure 4j,k), due to the valley thermal winds from more polluted sites, there were advective processes in the Xianyang airport. Moreover, as the role of the advective processes, the spatial–temporal evolution of relative humidity was not consistent with the BL. In other months, during the hours from 8:00 to 10:00, the relative humidity within the BL was relatively high, while the BLH was relatively low. Moreover, from 10:00 to 14:00, as the BLH gradually increased, the relative humidity within the BL gradually decreased with time. Subsequently, from 16:00 to 18:00, the relative humidity within the BL increased gradually as the BLH decreased with time. One explanation is that, as the water vapor within the BL was fully mixed due to turbulent flow, the space for water vapor to min became larger with the increasing BLH, and the water vapor was diluted; correspondingly, the relative humidity gradually decreased. As seen in Figure 4, the values of relative humidity within the BL were all relatively small. As the height increased, the relative humidity also tended to increase; moreover, the relative humidity within the BL was generally smaller than that above the BL. This may be because when there is low water vapor in the atmosphere (low relative humidity), the vertical variation in specific humidity within the BL is small, so the relative humidity gradually increases with height as the temperature decreases with height (Figure 3).
Overall, the relative humidity within the BL gradually decreased with the increasing BLH during the haze events at Xianyang Airport. However, as the BLH decreased with time, the relative humidity within the BL gradually increased. Moreover, in the vertical direction, the relative humidity within the BL gradually increased with height and was generally lower than that above the BL.

3.2. Statistical Characteristics of Haze

This study used data from 1230 haze and 60 no-haze events, all occurring between 2016 and 2021. These were detected by CFL and microwave radiometer to obtain high-resolution and accurate statistical characteristics of temperature, relative humidity (RH) and wind within the BL of the haze at Xianyang Airport, and then analyzed.

3.2.1. Statistical Characteristics of BLH during Haze Events

The BLHs of haze events and no-haze events were calculated using the C n 2 , the horizontal wind direction and wind speed detected by the CFL. Figure 5 shows the monthly average boundary layer heights of haze events ( BLH haze ) and no-haze events ( BLH no haze ), as well as the difference between BLH no haze and BLH haze (Figure 5c). As shown in Figure 5a, the BLH haze in June, July and August were higher than in other months at the same time, while the BLH haze in November, December, January, and February were lower than in other months at the same time. In the morning (8:00–9:00), low altitude with lower solar radiation characterized the stable boundary layer, and the atmospheric structure was very stable; moreover, the BLH haze was very small in this period, including 200 m in January and December, and 500 m in June and July. After 9:00, the BLH haze gradually increased with the rising of the sun and the continuous strengthening of solar radiation. For the period 13:00–15:00, the BLH haze reached the maximum (as shown by the black line in Figure 5a): the maximum BLH haze in December, January, and February was about 600 m, while the maximum BLH haze in June and July reached 1100 m, and the maximum BLH a in other months was between 600 m and 1000 m. After 15:00, the BLH haze gradually decreased with the continuous weakening of solar radiation. Subsequently, the BLH haze gradually decreased again to 500 m at 18:00. As shown in Figure 5, the characteristics of BLH haze and BLH no haze were consistent with time; however, the BLH haze was lower than BLH no haze , with a minimum difference of 150 m in January, and a maximum difference of 300 m in July (as shown in Figure 5c).
In short, the BLH haze of the haze at Xianyang Airport was generally less than 1000 m, and this was also less than the BLH no haze , which indicates that the lower BLH was more favorable for the development of the haze. Moreover, the BLH haze in December and January was distributed at 200–600 m lower than other months while that in June and July was distributed at 500–1100 m higher than other months and the maximum BLH a appeared at 13:00–15:00.

3.2.2. Statistical Characteristics of Temperature within the BL during Haze Events

Figure 6 illustrates the time distribution of the average temperature within the BL of the haze events ( Ta hzae ) and no-haze events ( Ta no hzae ). The time distribution of sensible heat flux(the average 100 m vertical temperature difference Δ T haze and Δ T no haze ) within the BL of haze events and no-haze events were calculated (Figure 6b,d) according to Equation (6), in which h 1 and h 2 are two adjacent heights ( h 1 > h 2 ), and correspond to the temperatures T h 1 and T h 2 .
{ Δ T = ( T h 1 T h 2 ) / Δ h Δ h = ( h 1 h 2 ) / 100
As shown in Figure 5a and Figure 6a, in the morning (8:00–9:00), the Ta haze was lower than at other times, with the corresponding BLH haze also being lower than at other times. After 9:00, as the sun rose and the Ta haze began to increase, the heat flux gradually increased; meanwhile, the corresponding BLH haze also gradually increased. Furthermore, during the period 13:00–15:00, the Ta haze reached its maximum, with the corresponding BLH haze also reaching its maximum. However, the Ta haze began to decrease, with the BLH haze decreasing gradually after 16:00. Until 18:00, the Ta haze clearly fell and the corresponding BLH haze fell to 500 m. In addition, for the same time (same abscissa in Figure 6a), the months with a larger T a (June, July, and August) correspond to the higher BLH haze , while the months with a lower T a (January, February, and December) correspond to the lower BLH haze . These correlations indicate that the changes in low-level temperature exert a strong influence on the development of the BLH. When the temperature increased, the low-altitude energy interaction intensified, which led to the enhancement of turbulent motion and promoted the development of BLH. However, when the temperature decreased, the low-level energy interaction weakened and the turbulent motion also decreased, which suppressed the development of BLH. Comparing Figure 6a,c, it is seen that the characteristics of Ta haze and Ta no haze are consistent with time; moreover, Ta haze was larger than Ta no haze during the months except September, in which the haze events always occurred after precipitation that led to the Ta haze being lower than the Ta no haze . As shown in Figure 6e, the maximum difference between Ta haze and Ta no haze was 6 °C in February, and the min difference in Ta haze   and   Ta no haze was less than 1 ℃ in August.
As shown in Figure 6b, the Δ T haze was mainly distributed in the range of −0.9 °C–0.4 °C. In the morning (8:00–9:00), the Δ T haze within the BL was greater than 0 °C in January, February, November, and December, with an inversion layer at low altitude; meanwhile, the Δ T haze was also very small (less than −0.2 °C) in the other months. This indicates that the low altitude was very stable. Meanwhile, the atmospheric structure was a stable BL during this period. Furthermore, after 9:00, due to the continuous heating of the ground temperature, the temperature inversion layer disappeared and the Δ T haze within the BL began to grow; meanwhile, the low altitude changed from a stable BL to a mixed BL. Moreover, between 13:00 and 15:00, the Δ T haze within the BL reached a maximum (−0.9 °C in June, July, and August, and about −0.4 °C in January and December) with the heat mining effect reaching the maximum, and the corresponding BLH also reaching its maximum. After 16:00, the Δ T haze within the BL gradually decreased with the heat mining effect at low altitude becoming weaker, and the BLH also gradually decreased. Comparing Figure 6b,d,f, it can be observed that Δ T haze was lower than Δ T no haze ; moreover, the maximum difference in Δ T haze   and   Δ T no haze was 2 ℃ in June, and the min difference in Δ T haze   and   Δ T no haze was less than 0.2 ℃ in August. These results indicate that the sensible heat flux of the haze was less than that of the no-haze, and the atmospheric structure for the haze was more stable than that for no-haze.
Overall, the Ta haze was larger than the Ta no haze , and the Δ T haze at low altitude was smaller than the Δ T no haze . Meanwhile, the atmospheric structure for haze events was more stable than that for no-haze events.

3.2.3. Statistical Characteristics of Relative Humidity within the BL during Haze Events

Figure 7 shows the distributions of the average relative humidity ( RH haze and RH no haze ), and the average 100 m vertical relative humidity difference ( Δ RH haze and Δ RH no haze ) within the BL. As shown in Figure 7a,c, it can be observed that the RH haze of haze events at Xianyang Airport was generally lower than 65% and higher than RH no haze , except in July. As shown in Figure 7e, the maximum difference in RH haze and RH no haze was 20% in September, and the min difference in RH haze and RH no haze was less than 5% in June. Moreover, the RH haze was distributed between 20% and 40% in January and February, while the RH haze was distributed between 40% and 65% in July, August, and September. During late autumn and winter, Xianyang Airport was under the control of a weak high ridge, with a stable atmospheric structure and little precipitation, so the was low. However, the haze events at Xianyang Airport mostly occurred after precipitation during the autumn, so the RH haze was higher. In terms of temporal variability, the RH haze was higher in the morning (8:00–9:00) than at other times, and the corresponding BLH was lower and the air pollution was more serious. After 9:00, the RH haze decreased gradually with increasing BLH due to the strengthening of the mixing effect and the dilution of water vapor. For the period 13:00–15:00, the RH haze decreased to a minimum, with the BLH reaching a maximum. After 17:00, there was some increase in the RH haze within the BL. In short, the larger the relative humidity, the lower the BLH, with more serious air pollution.
As shown in Figure 7b, the Δ R H h a z e in January, February, November, and December was distributed in the range of −1~1%, and that in March, April, May, and October was distributed in the range of 0~1.5%; the Δ R H h a z e in June, July and August was distributed in the range of 1.5~3%. As shown in Figure 7f, the Δ R H h a z e was lower than the Δ R H n o h a z e , which indicates the water vapor interaction in the haze events was less than that in the no-haze events. In the morning (8:00–9:00), the Δ R H h a z e was smaller than at other times. After 9:00, the Δ R H h a z e increased gradually as the BLH increased, reaching its maximum at 13:00–15:00; subsequently, the Δ R H h a z e gradually decreased after 16:00. Comparing Figure 6b and Figure 7b, it is observed that the Δ R H h a z e varied in the opposite manner to the Δ T h a z e , in that the Δ R H h a z e was negative, while the Δ T h a z e was positive at 8:00–9:00 in January, February, November, and December. Moreover, Δ R H h a z e in other months had a small positive value, while the corresponding had a small negative value during this period. It is possible that the specific humidity within the BL varied little with height; furthermore, when the temperature gradually increases (decreases) with height, the corresponding relative humidity will gradually decrease (increase) with height.

3.2.4. Statistical Characteristics of Wind within the BL during Haze Events

Figure 8 shows the average horizontal wind speed and wind direction within the BL during the haze events and no-haze events in different months. It is observed in Figure 8a that the average wind speed within the BL was less than 4 m/s during haze events and did not vary much with time, which was conducive to the development of haze.
Comparing Figure 8a,b, it can be seen that w i n d   s p e e d h a z e was lower than w i n d   s p e e d n o h a z e , and w i n d   d i r e c t i o n h a z e was consistent with w i n d   d i r e c t i o n n o h a z e . Moreover, the maximum difference between w i n d   s p e e d h a z e and w i n d   s p e e d n o h a z e was 4 m/s in November, and the minimum difference was 2 m/s in August (shown in Figure 8c). These results indicate that the low-level turbulence of the haze events was less than that of the no-haze events. Due to the cold air from the north, the dominant wind direction was generally northeaster in December, January, February, and March; moreover. Due to the warm air from the south, the dominant wind direction was generally southeaster or southwester in April, May, June, July, and August. However, in September and October, the dominant wind direction was northeaster or west and the wind speed was very weak due to there was not obvious cold or warm air. Meanwhile, from 8:00 to 11:00, the wind direction changed little with time, indicating that the atmospheric turbulent motion was small and the corresponding BLH was also low. Furthermore, after 16:00, the average horizontal wind direction varied little with time, and the atmospheric structure became relatively stable, with the corresponding BLH about 500 m.

3.3. The Relationship between Haze BLH and the Atmospheric Environment

3.3.1. The Relationship between Haze BLH and AQI

To further analyze the relationship between the haze BLH and air quality, the AQI of 1230 haze events were classified and then averaged by time to obtain Figure 9. Comparing Figure 5 and Figure 9, during December, January, and February—months with a low BLH haze , the average AQI was distributed in the range of 140~190 and the air pollution was severe; however, during June, July, and August—months with a high BLH haze , the average AQI was distributed in the range of 70~100 with lighter air pollution. In short, the months with a lower BLH haze correspond to larger average AQI.
In the morning (8:00–9:00), due to the stable atmospheric structure with the low BLH, the average AQI was relatively high and the air pollution was severe. Moreover, during the period from 9:00 to 12:00, the average AQI slowly decreased with the continuously increasing BLH. From 12:00 to 15:00, as the BLH reached its maximum, the atmospheric turbulence movement was relatively intense and the average AQI fell rapidly, which was conducive to the dissipation of the haze and better air quality. After 16:00, as the BLH gradually decreased, the average AQI did not change much with time, and the air quality was very good.
Overall, the larger the average AQI, the worse the air quality and the more severe the air pollution; meanwhile, the corresponding BLH was lower and the atmospheric structure was more stable. However, when the BLH became progressively higher with time, the average AQI became progressively smaller, and the air quality progressively improved.

3.3.2. The Relationship between Haze BLH and PM 2.5 and PM 10

To reveal the relationships between BLH, PM 2.5 and PM 10 during the haze events, we obtained the average temporal distributions of PM 2.5 and PM 10 (shown in Figure 10). As shown in Figure 10, the trends for the average PM 2.5 and PM 10 with time were consistent. In January, with the lowest BLH, the average PM 2.5 was distributed from 100 μ g · m 3 to 140 μ g · m 3 , and the average PM 10 was distributed from 180 μ g · m 3 to 260 μ g · m 3 , both being larger than in the other months. However, in July with the highest BLH, the average PM 2.5 was distributed from 40 μg·m−3 to 60 μ g · m 3 , and the average PM 10 was distributed from 70 μ g · m 3 to 90 μ g · m 3 , both being lower than in the other months. In short, the average PM 2.5 and PM 10 of the month with the higher BLH haze (Figure 5a) and higher T a h a z e (Figure 6a) were lower than those of the other months at the same time (the same abscissa in Figure 10).
Comparing Figure 5 and Figure 10, the average PM 2.5 and PM 10 demonstrate opposite trends to the BLH haze with time. In the morning (8:00–9:00), the stable atmospheric structure with the low BLHhaze was prone to the accumulation of pollution, which led to the average PM 2.5 and PM 10 being larger than those for other periods. After 9:00, the average PM 2.5 and PM 10 decreased gradually with the increasing BLH haze . Furthermore, between 13:00 and 15:00, the BLH haze reached its maximum, thereby producing more space for pollutant mixing and dilution, so the average PM 2.5 and PM 10 were reduced. However, there were small changes in the average PM 2.5 and PM 10 after 16:00. Overall, the lower the BLH, the more stable the atmospheric structure and the larger the average PM 2.5 and PM 10 ; however, the more serious was the atmospheric pollution.

4. Discussion

The bulk Richardson number-based method (Ri) used in ERA5 is widely used to detect a “well-mixed” BLH [42,43]; however, the Ri is unable to accurate determine the BLH when the atmospheric layer is not well-mixed. Hence, the ERA5 BLH can be used to verify the method used in our study for the period 12:00–16:00 BT.
In this study, we combined the C n 2 , and horizontal wind speed and direction to create a method of determining the BLH, considering temperature, RH, and wind. Meanwhile, the adjust parameter ( α in Equations (4) and (5) assumed a different value based on whether the low-level atmospheric layer was well-mixed or not. By comparing against ERA5, our method is basically shown to be credible for the well-mixed BLH. Meanwhile, our method is also credible theoretically, when there is a strong wind shear around the not-well-mixed BLH. Based on previous studies [40,41], there are wind shears around the BLH in the most cases. Overall, the BLHs retrieved by our method are basically credible.

5. Conclusions

In this study, the combined data detected by using a wind-profiling radar, microwave radiometer and atmospheric particulate monitor during 1230 haze events and 60 no-haze events, occurring at Xianyang Airport, were analyzed. The main conclusions are as follows:
(1)
The BLH haze was generally lower than 1000 m and the BLH no haze ; moreover, the lower BLH haze in December and January was distributed in the range of 200–600 m, while the higher BLH haze in June and July was distributed in the range of 500–1100 m; meanwhile, the max BLH haze appeared at 13:00–15:00.
(2)
When the Ta haze was higher, the heat interaction was stronger, the turbulent motion of the atmosphere was more intense and the corresponding BLH was higher. Conversely, when the Ta haze was lower, the heat interaction between ground and air quality was weaker; moreover, the atmospheric structure was more stable and the corresponding BLH was lower.
(3)
When the BLH rose, the RH haze gradually decreased, and the RH haze gradually increased with height; conversely, when the BLH decreased, the RH haze gradually increased; moreover, the larger the RH, the lower the BLH, and the more serious the air pollution.
(4)
Due to the relatively stable atmospheric structure with the low BLH, the average AQI, PM 2.5 and PM 10 , were large, the air quality was poor, and the air pollution was severe. However, when the BLH gradually became higher with time, the average AQI, PM 2.5 and PM 10 , gradually decreased and the air quality gradually improved.

Author Contributions

Conceptualization, H.M. and M.W.; methodology, H.M.; software, L.G.; validation, M.G.; formal analysis, Y.Q.; investigation, M.G.; resources, L.G.; writing—original draft preparation, H.M.; writing—review and editing, A.C. and M.G.; language, A.C. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by the project ZR2021QD041 and ZR2020MD052 supported by Shandong Provincial Natural Science Foundation; the project of Xinjiang scientific and technological innovation team (Tianshan innovation team).

Data Availability Statement

Not applicable.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. (a) Location map of Xianyang International Airport; (b) the CFL-03 wind profiling radar; (c) the microwave radiometer.
Figure 1. (a) Location map of Xianyang International Airport; (b) the CFL-03 wind profiling radar; (c) the microwave radiometer.
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Figure 2. Comparison of BLHs (black line) inversed by CFL and BLHs (black circle) from ERA-Interim; (a) 8:00–18:00 on 4 November 2016; (b) 8:00–18:00 on 4 March 2021; (c) no-haze event 8:00–18:00 on 3 November 2021.
Figure 2. Comparison of BLHs (black line) inversed by CFL and BLHs (black circle) from ERA-Interim; (a) 8:00–18:00 on 4 November 2016; (b) 8:00–18:00 on 4 March 2021; (c) no-haze event 8:00–18:00 on 3 November 2021.
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Figure 3. Spatial–temporal evolutions of temperature and horizontal wind during typical haze events; the blue lines are the BLHs with time.
Figure 3. Spatial–temporal evolutions of temperature and horizontal wind during typical haze events; the blue lines are the BLHs with time.
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Figure 4. Spatial–temporal evolutions of relative humidity during typical haze events; the black line is the variation in BLH with time.
Figure 4. Spatial–temporal evolutions of relative humidity during typical haze events; the black line is the variation in BLH with time.
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Figure 5. (a) Temporal distribution of the BLH haze in different months; the black line indicates the time of the highest boundary layer. (b) The temporal distribution of the BLH no haze in different months. (c) Differences in the BLH no haze and BLH haze .
Figure 5. (a) Temporal distribution of the BLH haze in different months; the black line indicates the time of the highest boundary layer. (b) The temporal distribution of the BLH no haze in different months. (c) Differences in the BLH no haze and BLH haze .
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Figure 6. Temporal distribution of average temperature within the BL during (a) the haze events Ta haze , (c) the no-haze events Ta no haze ; the distribution of monthly average sensible heat fluxwithin the BL during (b) the haze events Δ T haze ; (d) the no-haze events Δ T no haze in different months; (e) the difference of the Ta no haze and Ta haze ; (f) the difference of the Δ T no haze and Δ T haze .
Figure 6. Temporal distribution of average temperature within the BL during (a) the haze events Ta haze , (c) the no-haze events Ta no haze ; the distribution of monthly average sensible heat fluxwithin the BL during (b) the haze events Δ T haze ; (d) the no-haze events Δ T no haze in different months; (e) the difference of the Ta no haze and Ta haze ; (f) the difference of the Δ T no haze and Δ T haze .
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Figure 7. Temporal distribution of average relative humidity within the BL during (a) the haze events RH haze and (c) the no-haze events RH no haze ; the distribution of monthly average vertical relative humidity difference within the BL during (b) the haze events Δ RH haze and (d) the no-haze events Δ RH no haze in different months; (e) the difference in the RH no haze and RH haze ; (f) the difference in the Δ RH no haze and Δ RH haze .
Figure 7. Temporal distribution of average relative humidity within the BL during (a) the haze events RH haze and (c) the no-haze events RH no haze ; the distribution of monthly average vertical relative humidity difference within the BL during (b) the haze events Δ RH haze and (d) the no-haze events Δ RH no haze in different months; (e) the difference in the RH no haze and RH haze ; (f) the difference in the Δ RH no haze and Δ RH haze .
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Figure 8. Temporal distribution of average horizontal wind within the BL per half hour during (a) the haze events W i n d h a z e and (b) the no-haze events W i n d n o h a z e in different months; (c) the difference in the W i n d   S p e e d n o h a z e   and W i n d   S p e e d h a z e   .
Figure 8. Temporal distribution of average horizontal wind within the BL per half hour during (a) the haze events W i n d h a z e and (b) the no-haze events W i n d n o h a z e in different months; (c) the difference in the W i n d   S p e e d n o h a z e   and W i n d   S p e e d h a z e   .
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Figure 9. The temporal distribution of the average AQI during haze events in different months.
Figure 9. The temporal distribution of the average AQI during haze events in different months.
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Figure 10. (a) The temporal distribution of average PM 2.5 during haze events in different months; (b) The temporal distribution of average PM 10 during haze events in different months.
Figure 10. (a) The temporal distribution of average PM 2.5 during haze events in different months; (b) The temporal distribution of average PM 10 during haze events in different months.
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Table 1. Parameters of CFL-03 boundary layer wind profiling radar.
Table 1. Parameters of CFL-03 boundary layer wind profiling radar.
Parameter NameParameterParameter NameHigh-ModeLow-Mode
Radar wavelength227 mmPulse width0.66 μs0.33 μs
Beam widthHeight resolution12060
Beam number5FFT points512256
Antenna gain25 dBReceiver band width1.5 MHz3.0 MHz
Feeder loss2 dBMin detection altitude60060
Peak transmitted power2.36 KWNumber of coherent accumulations64100
Noise coefficient2 dB
Table 2. The monthly haze events at Xianyang Airport from 2016 to 2021.
Table 2. The monthly haze events at Xianyang Airport from 2016 to 2021.
YearJanFebMarAprMayJuneJulyAugSepOctNovDec
2016272825231310162318142430
201729262113101381113132531
20182626251211911148162329
2019312818161094816182326
2020262419208913511101822
20212319201285595122125
Sum16215112896605557707183134163
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Ming, H.; Wang, M.; Gao, L.; Qian, Y.; Gao, M.; Chehri, A. Study on the Boundary Layer of the Haze at Xianyang Airport Based on Multi-Source Detection Data. Remote Sens. 2023, 15, 641. https://doi.org/10.3390/rs15030641

AMA Style

Ming H, Wang M, Gao L, Qian Y, Gao M, Chehri A. Study on the Boundary Layer of the Haze at Xianyang Airport Based on Multi-Source Detection Data. Remote Sensing. 2023; 15(3):641. https://doi.org/10.3390/rs15030641

Chicago/Turabian Style

Ming, Hu, Minzhong Wang, Lianhui Gao, Yijia Qian, Mingliang Gao, and Abdellah Chehri. 2023. "Study on the Boundary Layer of the Haze at Xianyang Airport Based on Multi-Source Detection Data" Remote Sensing 15, no. 3: 641. https://doi.org/10.3390/rs15030641

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