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--> --> --> -->2.1. Site, instruments, and measurements
Measurements were executed during daytime [0500–2000 LST(LST=UTC+8)] from 2 August to 28 September 2017 over a summer maize (Zea mays) field at the Yucheng Comprehensive Experimental Station, Chinese Academy of Sciences (36°57’N, 116°36’E; 36 m MSL). During the experiment periods, the maize was in the flourishing stage and its height was constant. The site was located in the Yellow River alluvial plain of the North China Plain, Shandong Province, China. The surface soil texture at the station was that of a silty loam with moderate salinity and alkalinity. The experimental site was fairly flat, and the fetch requirements for flux measurements were well satisfied within 200 m of the instrument locations. During the observation period, the mean crop height was 2.2 m.Gradient measuring sensors and EC instruments were installed at two masts separated by a horizontal distance of approximately 3 m. For gradient measurements, all sensors or air sampling inlets were mounted at 4.70 m and 3.15 m. Two temperature and relative humidity sensors (HMP155A, Vaisala, Finland) were housed in special radiation shields. Wind speeds were measured with two 2D ultrasonic wind sensors (WMT700, Vaisala, Finland). The two-height O3 concentrations were measured with a slow-response UV photometric O3 analyzer (Model 205, 2B Technologies Inc., USA; hereafter referred to as M205). Its measurement precision is 1.0 ppb, with a resolution of 0.1 ppb. By using two solenoid valves, two-level air samples were cyclically (switching once per 5 min) drawn down into an analyzer with two separate inlet lines (PTFE Teflon) that were 5.5 m long with 4-mm inner diameters.
The EC O3 flux was measured in combination with observations from the Chinese Terrestrial Ecosystem Flux Observational Research Network (or ChinaFLUX). The instrumentation included a 3D sonic anemometer (CSAT3, Campbell Scientific Inc., USA) and an open-path CO2/H2O gas analyzer (LI-7500, LI-COR, Nebraska, USA) for measuring sensible heat, latent heat, and CO2 fluxes. The O3 fluctuation (in mV) was measured with a closed-path fast-response O3 analyzer that was cooperatively developed by Karlsruhe Institute of Technology and Enviscope GmbH (Germany) (Zahn et al., 2012; hereafter referred to as ENVI). Air was drawn down through a 4.5-m-long tube with a 4-mm inner diameter at a flow rate of 2.4 l min?1 and passed over a small disc coated with O3-sensitive dye. Its output signal (in mV) was positively correlated with the ambient O3 concentration (Muller et al., 2010). Because of the continuous consumption of O3-sensitive dye, we replaced the dye disc every 3–4 days, approximately. Radiation variables were also measured, including net radiation (CNR1, Kipp & Zonen, The Netherlands) and photosynthetically active radiation (LI-190SB, LI-COR, Nebraska, USA). All radiation and EC sensors were installed at a height of 3.5 m.
All gradient measurements were sampled with a frequency of 0.1 Hz, and the averages for every 5 min were recorded by a data-logger (CR3000). All high-frequency vector and scalar raw data were continuously sampled and stored using a SMARTFlux system (LI-COR, Nebraska, USA) with a frequency of 10 Hz.
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2.2. Gradient methods
According to Fick’s first law, the scalar flux in the constant-flux layer can be expressed as the product of the vertical concentration gradient (Usually, the gas concentration vertical gradient is obtained by directly measuring concentrations at two or more layers with one or more gas analyzer(s), while Kc is obtained from other measurements. Based on MOST, the eddy diffusivity for O3 can be assumed to be equal to the diffusivity for momentum, heat, water vapor, and trace gases. To assess the differences in the calculated Kc from using the different methods, three methods were selected in the present study, as briefly described below.
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2.2.1. Aerodynamic gradient method
The first method, the aerodynamic gradient (AG) method, is based on the gradients of temperature, wind speed, and gas concentrations. As the two measurement heights of three variables are the same, the AG method O3 flux can be calculated as (Bocquet et al., 2011):where
where the Richardson number (Ri) is estimated by:
where g is the gravitational acceleration (9.8 m s?2), Δθ is the potential temperature gradient, and Δzu and Δzθ are the height differences in the wind speed and temperature, respectively. As the mean air pressure is very close to 1000 hPa, the potential temperature was replaced with the air temperature.
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2.2.2. AG method combined with EC measurements
Since the EC system was employed in this experiment, the u* and H can be obtained directly. Therefore, the Kc can be calculated using the universal flux–gradient relationships method (Businger et al., 1971). The O3 flux calculated with this AG method with EC measurements (hereafter referred to as the AGEC method) can be written as (Rinne et al., 2000):where the u* and Obukhov length L are taken from the EC measurements.
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2.2.3. MBR method
Based on the measurements of fluxes (momentum, sensible heat, and latent heat fluxes) and gradients (wind speed, temperature, and relative humidity), three MBR exchange coefficients could be calculated. In this study, the exchange coefficient with the MBR method was based only on the H and temperature gradient, and the O3 flux for MBR was calculated as (Walker et al., 2006):where w is the vertical wind speed (m s?1),
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2.3. EC O3 flux calculation
As the ENVI’s output is a relative measure of the O3 concentration, and its stability is affected by the consumption of O3-sensitive dye and environmental conditions, it must simultaneously calibrate. In this study, the “ratio method” was used to calibrate the ENVI’s signal-output (X), meaning that X (in mV) is proportional to the absolute ambient O3 concentration over a 30-min period (Muller et al., 2010). Based on this assumption, the O3 deposition velocity (Vd), defined as the O3 flux divided by the O3 concentration, can be calculated by:where the role of the minus sign in Eq. (8) is to maintain a positive Vd, because the O3 flux is always directed downward (negative). The raw EC O3 flux,
where
In practice, the O3 flux and other EC data were processed by EddyPro? software (LI-COR, NE, USA) with a series of corrections. The double rotation method was used to correct the error due to non-level terrain (Wilczak et al., 2001). Ozone flux loss caused by time delay was corrected by the maximum covariance method (Moncrieff et al., 1997). The frequency response attenuation due to tubing was corrected using methods described by Ibrom et al. (2007). The Webb-Pearman-Leuning (WPL) correction (Webb et al., 1980) term only considered density variations caused by water vapor (Zhu et al., 2015).
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3.1. Comparison of the exchange coefficients from different methods
Exchange coefficients (K) are key factors for gradient method fluxes. Different methods of determining K result in different exchange coefficients. Figure 1 shows the mean diurnal variations of the transfer coefficients calculated by the three methods. Overall, the variation trends in the three K types are the same, presenting an obvious diurnal variation pattern. With the increase in radiation and temperature, the air turbulence becomes strong, and the three K types are increased. Around noon, the maximum K appears with smooth changes. It starts to decrease in the later afternoon. However, large differences exist in the three K values. The K value determined by the AG method (KAG) is the largest, and the K calculated with the MBR method (KMBR) is the smallest.Figure1. Diurnal variations of the K calculated by the MBR, AGEC and AG methods.
The KAGEC value is between those of KMBR and KAG, and the variables for calculating KAGEC are measured by the EC technique. It can therefore be considered the most appropriate, as validated by comparing its results with those of the EC O3 flux (see section 3.3). The 30-min averaged KAG and KMBR are compared with KAGEC in Fig. 2. Based on the scatterplot, coefficient of determination (R2), and significance level, it is clear that the correlation between KMBR and KAGEC is better than that between KAG and KAGEC. Based on the linear regression equations, KMBR is approximately 0.08 m s?1 lower than the KAGEC in value, while the KAG is larger than the KAGEC overall. The difference becomes small when K is large. The mean values of KAGEC, KMBR, and KAG are 0.20, 0.12, and 0.25, respectively. KMBR is 40% lower and KAG is 25% higher than KAGEC.
Figure2. Comparison of the 30-min K computed with the MBR, AGEC and AG methods.
The differences in the exchange coefficients are affected by their calculation equations and the accuracy of each variable measurement. The large differences in the K values show that there were systematic errors in determining K with the different methods (see Fig.2). For KMBR, the error sources include the H and temperature gradient measurements. Wilson et al. (2002) evaluated the energy balance closure of 22 sites in FLUXNET and concluded that a general lack of closure existed at most sites, with a mean imbalance in the order of 20% in most conditions. The sum of the measured H and LE (latent heat flux) with the EC method, (H + LE)EC, is smaller than the difference in net radiation (Rn) and soil heat flux (G) (Rn?G). This may imply that the H measured with EC might be underestimated, leading to the underestimation of KMBR. Additionally, the error in the temperature gradient is dependent on the sensors’ performance. Although the best precision that the temperature sensors can reach is ±0.055°C, as the two temperature sensors were not exchanged periodically, a radiation shield could also result in a certain systematic bias in the temperature at the two levels (Loubet et al., 2013). To eliminate the systematic error of two temperature sensors, using thermocouples rather than the routine temperature sensors may be a good choice. It would be better if two temperature sensors could be exchanged regularly.
The sources of error and uncertainty in KAG come from the wind speed measurements, estimations of d, parameters of stability correction functions, etc. Wind speeds were measured with two new 2D sonic anemometers. The precision is ±0.1 m s?1 or 2% of the readings, and the initial wind speed is 0.01 m s?1 (according to the manual). We can consider the accuracy to be sufficiently high and the random error to be very limited. These assumptions would ensure that the wind speed gradient is reliable. Improper stability correction functions in Eq. (2) might also be error sources. The commonly used universal models and parameters of the functions are usually based on previous literature that utilized empirical equations obtained at a specific site and in a specific condition. Different researchers have presented different stability correction models and parameters (Foken, 2006; Song et al., 2010).
The error and uncertainty of zero-plane displacement (d) are dependent on the estimation method and parameters (Loubet et al., 2013). The commonly used method is simply estimated by the plant height (hc) being multiplied by a constant (usually in the range of 0.6–0.8). The second method is inversely derived from the flux–gradient relationships, and the scalar flux can utilize the EC measurements. The third method is estimated by linearly fitting the wind speed profiles U(z) and ln(z–d), making the root-mean-square error of the wind speed minimal in neutral conditions or making some corrections under non-neutral conditions. In this study, it was calculated as d = 0.67hc. To validate whether this is suitable, we compared the u* calculated by the third method (
Figure3. Comparison of u* measured with the EC technique and AG method.
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3.2. O3 concentration gradient
Figure 4 shows the frequency distribution of the O3 gradient in the daytime during the observation period. Most gradients are distributed in the range between ?6 μg m?3 and 0 μg m?3, and the median of the gradient is ?3 μg m?3. As the two-level O3 concentrations were measured with the same analyzer, the systematic error caused by the analyzers can be ignored. However, the random error must still be considered. The uncertainty or relative error of the gradient depends on the magnitude of the real gradient that can be estimated by the ratio of the sampling errors (Figure4. Frequency distribution of the O3 concentration gradient.
Figure 5 shows the mean diurnal variations of the O3 concentration (average of two levels) and gradient during the entire observation period. The analyzer is a new product, and its precision can guarantee that the O3 concentration is reliable. Compared to the ambient absolute concentration, the vertical O3 gradient is very small within the ranges of several ppb. In the morning, the gradient shows increasingly larger trends. It is less than 2 μg m?3 in the early morning (before 0900 LST), implying that there may be large uncertainty during this period. The change in the mean gradient is relatively stable in the afternoon, with a mean gradient of 3.6 μg m?3, starting to decrease after 1900 LST.
Figure5. Mean diurnal variations of the O3 concentration (average of two levels) and gradients during the entire observation period.
In general, the negative effects of O3 on crops happen in the daytime and during high concentration conditions (Pleijel et al., 2007; Feng et al., 2015). This can be reflected by O3 concentration–based assessing indexes (Dingenen et al., 2009), such as M7 [the 7-h (0900–1600 LST) mean O3 concentration] and AOT40 (the accumulated hourly O3 concentration above a 40 ppbV threshold). The mean gradient was more than 2.4 μg m?3 in the later morning and afternoon at high O3 concentrations (Fig. 5), implying that the uncertainty of the gradient is relatively small during the times that O3 is affecting the ecosystem.
The accuracy of the O3 gradient is a key variable for the O3 flux measured with gradient methods. It depends on not only the analyzer’s performance but also the measurement and calculation methods. For example, the number of measuring heights is a source of uncertainty for the gradient. According to AG theory, the flux is proportional to the concentration changes with height. For only the two-level measurements, a few random errors in the O3 concentration could result in a large bias in the O3 gradient. Hence, measuring the concentration profiles at more heights would filter or smooth out the random error, and the gradient would be more stable.
Besides the number of measuring heights, it is noteworthy that the proper calculation method is very important for reducing bias in the O3 gradient. In this study, the two-level O3 concentrations were measured alternately (in 5-min intervals) with one analyzer, in which there exists a measuring order issue (i.e., which 5-min O3 concentration level is measured first during a 30-min period). A simple average of each of the O3 concentration levels might produce certain errors without considering the measuring order. Table 1 presents an example of 30-min averaged O3 mix ratio gradients with two calculation methods. In method I, the upper and lower 30-min O3 concentrations are the simple re-average of three 5-min measurements. As shown in Table 1, the upper concentrations were measured during 1000–1005 LST, 1010–1015 LST, and 1020–1025 LST on 21 August 2017. The lower concentration measurements were taken during 1005–1010 LST, 1015–1020 LST, and 1025–1030 LST on 21 August 2017. In method II, the gaps were first filled with the averages before and after the 5-min measured O3 concentrations, and there were six 5-min data points for each height, including three measured and three gap-filled data points. The gradient was then calculated as the difference between the two-height O3 concentrations.
Start Time (LST) | |||||||
1000 | 1005 | 1010 | 1015 | 1020 | 1025 | 1030 | |
${\rm C_O}_{_3} $_upper (5 min, ppb) | 58.66* | 61.78 | 63.83* | 65.87 | 65.99* | 66.10 | 66.19* |
${\rm C_O}_{_3} $_lower (5 min, ppb) | 57.77 | 60.78* | 63.79 | 64.54* | 65.28 | 65.21* | 65.14 |
Mean1_upper (30 min) | 64.58** | ? | ? | 64.58*** | ? | ? | ? |
Mean1_lower (30 min) | 62.28** | ? | ? | 64.74*** | ? | ? | ? |
Mean2_upper (30 min) | 63.70** | ? | ? | 64.96*** | ? | ? | ? |
Mean2_lower (30 min) | 62.89** | ? | ? | 64.12*** | ? | ? | ? |
ΔC1 (Lower ? upper) | ?2.30** | ? | ? | 0.15*** | ? | ? | ? |
ΔC2 (Lower ? upper) | ?0.81** | ? | ? | ?0.84*** | ? | ? | ? |
Notes: *no measurements, filled with the average of the measurements before and after 5 min; **averages of 1000–1030 LST; ***averages of 1005–1035 LST. Mean1 (Method I) is the average of real measurements during a 30-min period with three data points; Mean2 (Method II) is the average of measurements and gap-filled data during a 30-min period with six data points. ΔC1 and ΔC2 are the differences in the lower and upper O3 concentrations that are calculated with Mean1 and Mean2. |
Table1. An example of a comparison of different O3 mix ratio gradient calculation methods.
It is clear that there are large differences in the O3 gradients determined with the two methods (see ΔC1 and ΔC2 in Table 1). To demonstrate that method II is better than method I, we calculated the gradient of an offset of 5 min (i.e., 1005–1035 LST), in which the measuring order is changed. With method I, the O3 gradients of 1000–1030 LST (?2.30 ppb) and 1005–1035 LST (0.15 ppb) are largely variable and even result in a change of sign. However, the variation in the gradients of 1000–1030 LST and 1005–1035 LST calculated with method II is very small (?0.81 ppb and ?0.84 ppb).
Figure 6 shows the diurnal variations of O3 gradients calculated with two methods and time ranges on 15 August 2017. In method I, the difference of two 30-min averaged O3 gradients during different time ranges (5-min offset) is very large sometimes (see the two solid lines in Fig. 6). However, the difference with method II is obviously small (see the two dashed lines in Fig. 6). Even so, the difference means that there was still some uncertainty in the O3 gradient calculated with method II.
Figure6. Diurnal variations of 30-min averaged O3 gradients calculated with two methods and time ranges on 15 August 2017. M1A: Method I and start times are on the hour or half-hour; M1B: Method I but start times are 5-min delayed; M2A: Method II and start times are on the hour or half-hour; M2B: Method II but start times are 5-min delayed.
The main reason for this phenomenon is that the concentration changes in 5 min, and the O3 gradient is on the same order of magnitude (maximum several ppb). If the measuring time is not synchronous, the gradient would be affected by the changing trend of the O3 concentration. To ensure that both the upper and lower intakes measure the same air eddy, setting a quick switching time (e.g. ~1 min) may eliminate the phenomenon and improve the performance of the gradient system. Of course, if possible, the use of two analyzers and periodically exchanging the sample position to measure the O3 concentrations at two heights is better than using one analyzer to cyclically measure them (Meyers et al., 1996). This not only removes the systematic bias from the two analyzers but can also eliminate the errors caused by asynchronous sampling.
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3.3. Comparison of O3 fluxes measured with the EC and different gradient methods
Figure 7 presents the mean diurnal variations of the O3 fluxes with different methods. The disparities in the O3 fluxes with different methods were small in the morning and large in the afternoon. This is primarily because the gradient was relatively large in the afternoon (see Fig. 5). As the analyzer's random error is relatively small and stable, its effect on the O3 flux will decrease at a large gradient. Relatively, the O3 flux calculated by the AGEC method (Figure7. Mean diurnal variations of the O3 fluxes estimated by different methods. The top and bottom of the vertical lines represent the mean ± std.
Figure 8 shows comparisons of daytime O3 fluxes calculated by the EC method (
Figure8. Comparisons of 30-min O3 fluxes estimated by different gradient methods and the EC method’s flux.
A few previous studies compared the gradient O3 flux with that of the EC technique and found that the results varied. Muller et al. (2009) found that the O3 flux determined by the gradient method was larger than that of the EC technique at a grassland area. The transfer coefficient was derived by the wind speed gradient and EC momentum flux. It also showed a very large comparison scatterplot, with a slope of 1.19 and a poor R2 (0.15). The O3 flux with the AGEC method was similar to the results presented by Muller et al. (2009). Loubet et al. (2013) compared the O3 fluxes and deposition velocities (Vd) with AG methods and the EC technique over a maize field and showed that the AG method had a roughly 40% larger Vd than the EC technique. In this study, the AG O3 flux was calculated from the product of u* (calculated by the wind speed gradient with a stability correction) by a concentration scaling parameter
The errors of the gradient method’s fluxes come from the joint effects of the exchange coefficient and gradient. The theoretical basis of the gradient method is MOST, but it is limited to the homogeneous surface layer (or constant-flux layer) above the roughness sub-layer, and a range of |z/L|≤1~2 (Foken, 2006). The large discrepancy among the O3 fluxes with different methods may be related to the non-ideal conditions. For example, the sensors’ heights were not elevated enough, and the turbulent intensity was not always strong enough. Rinne et al. (2000) summarized the sources of uncertainty with AG methods for hydrocarbon flux measurements and presented the error estimate of gradient measurements, turbulent exchange coefficients, and parameterizations. The uncertainty caused by the gradient measurement was the largest. Loubet et al. (2013) also analyzed the potential errors in the AG method. They included the non-stationarity of the concentration changes, temperature errors caused by shields, roughness sub-layer correction issues, uncertainty in the displacement height estimation, etc. Based on this error source analysis, the most important error source was determined to be the gradient measurement. Decreasing the uncertainty in the O3 gradient is the key to more accurately estimating the O3 flux for gradient methods. Increasing the number of analyzers and measuring levels might reduce the errors in the O3 gradient. The gradient calculated using only the two-level O3 concentrations can easily produce random errors.