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Article

Gridded Assessment of Mainland China’s Solar Energy Resources Using the Typical Meteorological Year Method and China Meteorological Forcing Dataset

by
Zongpeng Song
1,
Bo Wang
1,
Hui Zheng
2,*,
Shuanglong Jin
1,
Xiaolin Liu
1 and
Shenbing Hua
1
1
National Key Laboratory of Renewable Energy Grid-Integration, China Electric Power Research Institute, Beijing 100192, China
2
Key Laboratory of Regional Climate-Environment Research for Temperate East Asia, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing 100029, China
*
Author to whom correspondence should be addressed.
Atmosphere 2024, 15(2), 225; https://doi.org/10.3390/atmos15020225
Submission received: 21 December 2023 / Revised: 1 February 2024 / Accepted: 7 February 2024 / Published: 14 February 2024
Browse Figures
Figure 1
<p>Schematic diagram of the TMY generation procedure. The five three-hourly variables shown at the top are from CMFD.</p> "> Figure 2
<p>Study domain. Blue lines denote the Yangtze and Huai Rivers. Black lines denote the province boundaries.</p> "> Figure 3
<p>China’s solar energy resources assessed using the TMY method for a thirty-year period (1991 to 2020). (<b>a</b>) annual global horizontal solar radiation, and (<b>b</b>) abundance grade of the solar energy resources. The definitions of the grades A, B, C, and D are described in <a href="#sec2dot3-atmosphere-15-00225" class="html-sec">Section 2.3</a>.</p> "> Figure 4
<p>Relative changes in the solar radiation estimates using the reference periods of different lengths. The changes are relative to the thirty-year period from 1991 to 2020: (<b>a</b>) 10 years from 2011 to 2020; (<b>b</b>) 20 years from 2001 to 2020; (<b>c</b>) 40 years from 1981 to 2020; and (<b>d</b>) 50 years from 1971 to 2020.</p> "> Figure 5
<p>Relative difference between the MYA and TMY methods in calculating annual solar radiation. The left panels present the spatial distribution, whereas the right panels present the probability distribution function (PDF).</p> "> Figure 6
<p>Seasonal radiation estimated with the TMY method for the thirty-year period (1991 to 2020). The values are fractions of the annual totals. (<b>a</b>) MAM for March, April, and May; (<b>b</b>) JJA for June, July, and August; (<b>c</b>) SON for September, October, and November; and (<b>d</b>) DJF for December, January, and February.</p> "> Figure 7
<p>Seasonal stability index and grade of the solar energy resource assessed using the TMY method for the thirty-year period (1991 to 2020). The seasonal stability index is defined as the ratio of the minimum monthly radiation to its maximum value. The stability grades A, B, C, and D are defined in <a href="#sec2dot3-atmosphere-15-00225" class="html-sec">Section 2.3</a>.</p> "> Figure 8
<p>Difference between the MYA and TMY methods in calculating seasonal solar radiation for the thirty-year reference period (1991 to 2020). The values are presented as the percentage of the annual solar radiation estimated using the TMY method (<a href="#atmosphere-15-00225-f003" class="html-fig">Figure 3</a>a).</p> "> Figure 9
<p>Difference in the seasonal stability index and grade between the MYA and TMY methods: (<b>a</b>) Difference of the MYA method relative to TMY; (<b>b</b>) Difference in the seasonal stability grade of the MYA method relative to TMY. Red denotes an upgrade (up arrow), whereas blue denotes a downgrade (down arrow); (<b>c</b>) Probability distribution function (PDF) of the difference in the seasonal stability index.</p> "> Figure 10
<p>Sensitivity of annual solar radiation to the considered meteorological variables. The three rows present the impacts of wind speed, air temperature, and dew point, respectively. The right panels present the probability distribution function of the relative differences corresponding to the left panels.</p> "> Figure 11
<p>Sensitivity of the seasonal stability index to the considered meteorological variables. The three rows present the impacts of wind speed, air temperature, and dew point, respectively. The right panels present the cumulative distribution function of the relative changes corresponding to the left panels. The lower and upper numbers in the right panels denote the CDFs of the area with negative and non-negative changes, respectively.</p> ">
Versions Notes

Abstract

:
The National Standard of China has recommended the typical meteorological year (TMY) method for assessing solar energy resources. Compared with the widely adopted multi-year averaging (MYA) methods, the TMY method can consider the year-to-year variations of weather conditions and characterize solar radiation under climatological weather conditions. However, there are very few TMY-based solar energy assessments on the scale of China. On the national scale, the difference between the TMY and MYA methods, the requirement of the data record length, and the impacts of the selection of meteorological variables on the TMY-based assessment are still unclear. This study aims to fill these gaps by assessing mainland China’s solar energy resources using the TMY method and China Meteorological Forcing Dataset. The results show that the data record length could significantly influence annual total solar radiation estimation when the record length is shorter than 30 years. Whereas, the estimation becomes stable when the length is greater or equal to 30 years, suggesting a thirty-year data record is preferred. The difference between the MYA and TMY methods is exhibited primarily in places with modest or low abundance of solar radiation. The difference is nearly independent of the examined data record lengths, hinting at the role of regional-specific weather characteristics. The TMY and MYA methods differ more pronounced when assessing the seasonal stability grade. A total of 7.4% of the area of China experiences a downgrade from the TMY relative to the MYA methods, while a 3.15% area experiences an upgrade. The selection of the meteorological variables has a notable impact on the TMY-based assessment. Among the three meteorological variables examined, wind speed has the most considerable impact on both the annual total and seasonal stability, dew point has the second most significant impact, and air temperature has the least. The results are useful for guiding future research on solar energy assessment in China and could be helpful for solar energy development planning.

1. Introduction

Solar energy is abundant, clean, and widely distributed. It is an important renewable energy source for decarbonizing the energy system. However, solar energy varies significantly in space and time [1,2,3]. Assessing the abundance and stability of solar energy resources on a national scale at a fine spatial resolution is essential for renewable energy development planning [3,4].
Plenty of studies have assessed the solar energy resources of China. To name a few, Tang et al. [5] compiled a set of high-accuracy in situ solar radiation observations and assessed the technical potential for solar photovoltaic generation in China. Shi et al. [6] retrieved the solar photovoltaic map of China using the Fengyun-4 geostationary satellite observations. Despite the differences in the data sources, these assessment depends on solely solar radiation data and calculate the solar energy resources as multi-year averages (MYA) of the data.
It has been well recognized that the variation of solar energy is predominantly due to weather conditions. Since weather systems have nonlinear impacts on surface solar radiation, the arithmetic average of solar radiation differs from that under representative weather conditions [7]. The typical meteorological year (TMY) method aims to address this issue, as shown in Table 1. The method consists of two steps: generation of a TMY that could characterize the representative weather conditions and assessment of solar energy resources based on the generated TMY [7,8,9,10,11,12,13,14].
The TMY method originates at the Sandia National Laboratories [15]. A TMY is a set of 12 months. Each month is selected from a set of multiple years in a place. The weather characteristics of each month are closest to the climatology of the site. The closeness of the weather is measured by the weighted average of the Finkelstein–Schafer statistics of multiple meteorological variables. The variables often include solar radiation, wind speed, air temperature, and dew point. Since its origin, the TMY method has an increasing number of variations [16,17,18,19,20,21]. While the variations make no difference in the use of the Finkelstein–Schafer statistics, they differ mainly in the considered meteorological variables and the weights in averaging the variables. The Sandia, Danish, and Festa–Ratto approaches are three widely adopted variations. The Sandia approach employs nine daily statistics of four meteorological variables: (1) the daily mean, maximum, and minimum air temperature; (2) the daily mean, maximum, and minimum air humidity; (3) the daily mean and maximum wind speed, and; (4) the daily mean global solar radiation [12,13,14,15,22]. The Danish approach uses seven daily statistics of six variables, including daily maximum and mean air temperature, mean relative humidity, mean wind speed, mean atmospheric pressure, sunshine duration, and global radiation [22]. The Danish approach also removes the seasonal cycle from air temperature and global radiation and normalizes the daily residuals with their respective standard deviation. The Festa–Ratto approach [23] uses five daily statistics of four variables, which are daily maximum and mean temperature, mean relative humidity, mean wind speed, and global radiation. Similar to the Danish approach, the Festa–Ratto approach removes the smoothed long-term monthly mean from the daily variables and normalizes the daily residuals using the standard deviation. Due to its simplicity, the Sandia approach is still the most widely used one.
The National Standard of China (GB/T 42766–2023) [24] has recommended the Sandia TMY method with slight modifications [9]. The method has been widely adopted for plot-scale assessment in various climate regimes [9,10,25,26]. However, studies on the scale of China are few. To our knowledge, Solargis may be the only assessment product yet [27]. TMYs are created using the European Centre for Medium-Range Weather Forecasts Reanalysis version 5 (ERA5) [28,29] and Integrated Forecast System (IFS) data. It is a commercial product (https://solargis.com (accessed on 20 December 2023)), and the details of the production methods are largely not disclosed.
Due to the inadequacy of published studies, several scientific questions remain unclear in the national-scale solar energy assessment: how is the TMY method compared with the MYA method; what is the requirement of the data record length (in other words, the length of the reference climatology); and what is the impact of the included meteorological variables on the assessment.
This study aims to answer these questions by providing a gridded assessment using the TMY method and the China Meteorological Forcing Dataset (CMFD) version 1.7 [30]. The dataset is based on ERA5, with the biases being corrected using in situ observations. The correction improves the accuracy of the estimation of the meteorological variables [31,32]. Consequently, CMFD would be more suitable than ERA5 (used by Solargis) in generating TMY for China.
The paper is organized as follows. Section 2 details the TMY method, the used dataset, the experimental settings, and the analysis method. Section 3 presents the results and discussion. Finally, Section 4 draws the conclusions.

2. Data and Methods

2.1. China Meteorological Forcing Dataset

The CMFD version 1.7 [30] is a long-term, gridded surface meteorological dataset of mainland China at a spatial resolution of 0.1° and a temporal resolution of 3 hours from 1951 to 2020. The dataset is created based on ERA5 [28,29]. Biases in the reanalysis are corrected using in situ observations. The observations are from the China Meteorological Administration (CMA) and the National Oceanic and Atmospheric Administration’s National Centers for Environmental Information (NOAA NCEI). Validation against independent observations suggests that the quality is reasonable and consistent across mainland China [30,31,32].
CMFD contains multiple surface meteorological variables, including 10-m wind speed, 2-m air temperature, specific humidity, surface air pressure, downwelling solar irradiance, downwelling longwave irradiance, and precipitation. These variables are sufficient to characterize the interannual variations of weather conditions while facilitating the TMY-based assessment of solar energy resources.

2.2. Typical Meteorological Year

We generated TMYs at each CMFD grid cell. Figure 1 shows the diagram of the generation procedure. The procedure mostly follows the National Standard of China (GB/T 42766-2023) [24].
First, dew point temperature ( T d ; K ) was calculated from the three-hourly CMFD records by solving the equation of partial water vapor pressure as follows.
P s ( T d ) = q p ϵ + ( 1 − ϵ ) q ,
where q and p are the specific humidity ( kg kg − 1 ) and surface air pressure ( Pa ) from the CMFD, respectively. ϵ = 0.622 is the ratio of water vapor’s molecular weight to the average dry air molecular weight. P s ( T ) is the relationship between saturation water-vapor pressure ( P s ; Pa ) and temperature (T; K ). The relationship can be written as follows [33].
P s ( T ) = exp ( 34.494 − 4924.99 T − 36.06 ) ( T − 168.16 ) 1.57 .
The values of CMFD-specific humidity could occasionally approach zero, leading to an exceptionally low dew point temperature. To reduce the impact of these abnormal values on the statistics such as the daily mean and minimum, a minimum dew point temperature was set as T d ≥ − 65 °C. The minimum dew point corresponds to the saturated water vapor pressure of 1.1 Pa .
Second, daily statistics (i.e., mean, maximum, and minimum) were calculated from three-hourly data for four meteorological variables. The four variables are the surface downwelling solar radiation, 2 m air temperature, 10 m wind speed, and dew point temperature. The first three were obtained directly from the CMFD.
Third, given a period that could span multiple years, monthly Finkelstein–Schafer statistic ( F y , m ) [34] was calculated for each month m and year y of the period and for each daily statistics X as follows [24].
F y , m = 1 n y , m ∑ i = 1 n y , m | S y , m ( X y , m , i ) − S m ( X y , m , i ) | ,
where n y , m is the number of days of the month m and year y, X y , m , i is the i-th daily value in ascending order.
S y , m is monthly cumulative distribution function for month m and year y. The calculation is similar to Equation (5).
S y , m ( X y , m , i ) = i − 0.5 n y , m .
S m is long-term cumulative distribution function for the month ( m = 1 , ⋯ , 12 ) of the year.
S m ( X ) = 0 , X < X m , 1 j − 0.5 n m , X m , j ≤ X < X m , j + 1 1 , X ≥ X m , n m ,
where n m is the number of the daily values in month m. The values are from all the years of the period. X m , j is the j-th value ( j = 1 , 2 , ⋯ , n m ) in ascending order.
Fourth, a monthly weighted average ( F ¯ y , m ) was calculated from the Finkelstein–Schafer statistics [24].
F ¯ y , m = w ( R mean ) · F y , m ( R mean ) + w ( T a , mean ) · F y , m ( T a , mean ) + w ( T d , mean ) · F y , m ( T d , mean ) + w ( W mean ) · F y , m ( W mean ) + w ( T a , max ) · F y , m ( T a , max ) + w ( T d , max ) · F y , m ( T d , max ) + w ( W max ) · F y , m ( W max ) + w ( T a , min ) · F y , m ( T a , min ) + w ( T d , min ) · F y , m ( T d , min ) ,
where w is the averaging weight. The symbols, R , T a , T d , and W , denote the surface downwelling solar irradiation, 2 m air temperature, dew point temperature, and 10 m wind speed, respectively. The suffixes mean , max , and min denote the daily mean, maximum, and minimum values, respectively. We used three sets of averaging weights in this study, as detailed in Section 2.3.
Finally, TMY was generated at each CMFD grid cell based on the weighted average of the Finkelstein–Schafer statistics ( F ¯ y , m ). For each of the 12 months (m) of the year, the year (y) with the lowest values was selected out from the period.

2.3. Experimental Settings and Analysis Methods

We conducted 11 experiments in China. Figure 2 shows the study domain, and Table 2 lists the experimental settings. The experiments differ in the assessing methods (i.e., TMY versus MYA) or the parameter settings. Experiment A is the baseline experiment. The experiment uses the TMY method described in Section 2.2. The averaging weights in the Finkelstein–Schafer statistics for the used meteorological variables conform to the China National Standard GB/T 37526-2019 [35]. The climatology is derived using thirty-year CMFD records from 1991 to 2020. Experiments B–E compare the length of the reference period. The lengths of the periods increase from ten (Experiment B) to 50 years (Experiment E) at a ten-year interval. Two pairs of experiments, F versus A and G versus H, are designed to reveal the difference between the TMY and MYA methods. The two pairs differ in the reference period length (i.e., 30 years and 10 years). Experiments I–K examine the impacts of the considered meteorological variables by excluding wind speed, air temperature, and dew point in sequence.
We calculated the annual total solar radiation from each experiment. The abundance of solar energy was characterized in five grades according to the China National Standard GB/T 42766-2023 [24]: A if the annual solar energy is above 6300 × 10 6 J m − 2 , B if it is between 6300 × 10 6 and 5040 × 10 6 J m − 2 , C if it is between 5040 × 10 6 and 3780 × 10 6 J m − 2 , and D if the annual solar energy is below 3780 × 10 6 J m − 2 .
We also calculated the seasonal stability index from each experiment and then classified the index into four grades. The stability index is defined as the ratio of minimum monthly solar radiation to the maximum value in the TMY. The four stability grades are assigned according to the China National Standard GB/T 37526-2019 [35]: A if the ratio is above 0.47, B if the ratio is between 0.36 and 0.47, C if it falls within 0.28–0.36, and D if the ratio is below 0.28.

3. Results and Discussion

3.1. Annual Solar Radiation

Figure 3 shows the spatial distribution of China’s solar energy resources estimated from Experiment A. The resources are the most abundant (grade A) in the Tibetan Plateau, southern Xinjiang, western Inner Mongolian Plateau, and western Sichuan province. These areas occupy 28% of the whole territory of China. 42% of China exhibits modest resources (grade B). The areas are located in northern Xinjiang, the eastern Inner Mongolian Plateau, eastern Gansu Province, northern Shaanxi Province, and major parts of Yunnan, Shanxi, Jilin, Liaoning, Hebei, Shandong, Taiwan, and Hainan. There are 29% of China that have relatively low resources (grade C). The areas are mainly located in the middle to lower Yangtze River basin and parts of the Northeast. Meager resources (grade D) are found at the junction of Chongqing and Guizhou, which covers about 1% of China. The estimates are generally consistent with previous studies in the places where in situ observations are available [36]. In comparison with the assessment using interpolated in situ data [37], a lower estimate was found in the Hexi Corridor, where in situ observations are sparse.
Figure 4 presents the relative difference between Experiments B–E to Experiment A. The ten-year estimates show a significant difference from the thirty-year ones in most areas of China. The 0.9, 0.95, and 0.99 quantiles of the absolute difference are 3.79%, 4.59%, and 6.55%, respectively. The significant discrepancy suggests that ten years may not be sufficiently long to assess solar energy resources. The longer the data records, the more stable the assessment. The twenty-year estimates are closer to the thirty-year estimates. The 0.9, 0.95, and 0.99 quantiles are reduced to 3.05%, 3.64%, and 4.90%, respectively. A longer period beyond 30 years yields marginal differences. The 0.9, 0.95, and 0.99 quantiles of the absolute difference between the thirty-year and forty-year estimates are 2.18%, 2.70%, and 3.83%, respectively. These values are almost half of those for the ten-year estimates. The marginal difference suggests that a thirty-year period is sufficient for the assessment. Interestingly, the fifty-year estimates show a larger deviation than the forty-year estimates. We speculate that the deviation is due to the inhomogeneity of the CMFD data before 1981. This period has few in situ observations and almost zero satellite observations to correct the biases in ERA5. Therefore, we focus on the thirty-year period from 1991 to 2020 (Experiment A) in the following analyses.
Figure 5 compares Experiment A versus F and Experiment G versus H. The comparisons reveal the difference between the TMY and MYA methods in estimating the annual total solar radiation. The probability distribution function of the differences is symmetric around zero. The absolute relative difference estimated using the thirty-year data from 1991 to 2020 is less than 2.69 (the 0.99 quantiles), with a median value of 0.6%. The difference is mainly exhibited in parts of Shaanxi, eastern Sichuan, Chongqing, and Guizhou, where the Southwest China vortex and topographic effects have a strong influence. The difference between the TMY and MYA methods does not show a strong dependency on the reference period length. The median value of the absolute difference is 0.6% for the 30 years (Figure 5b) and 0.7% for the 10 years (Figure 5d). However, the locations of the difference vary with the selection of the reference period. For the 10 years, from 2011 to 2020, in addition to the regions listed above, the lower Yangtze River basin, Guangxi, and parts of Heilongjiang also exhibited changes. The spatial distributions hint at the influence of the East Asia monsoon and the northeast China cold vortex. Despite the difference described above, the TMY and MYA methods are indistinguishable in classifying the solar energy resource abundance grade, with only 3.5% area of China having a different grade (1.85% for upgrade and 1.68% for downgrade).

3.2. Seasonal Variations

Figure 6 shows the seasonal solar radiation estimated from Experiment A. The seasonal radiation is presented as a fraction of the annual total for comparing values at different places across China. The radiation is largest in summer and smallest in winter. Across the whole study domain, the middle Yangtze River basin and the northern parts of northeast China, Inner Mongolia, and Xinjiang exhibit the highest radiation in summer and the lowest radiation in winter. In autumn, the fraction is nearly uniform, except for a slightly higher value in Guangdong and Guangxi and a marginally lower one in the northern part of northeast China. In spring, northern China shows a slightly higher seasonal fraction than southern China.
Figure 7 classifies the seasonal stability grade based on the seasonal radiation fraction shown in Figure 6. The stability grade is highest in Yunnan, western Sichuan, and southern Xizang. The areas where the winter-to-summer radiation ratio is above 0.47 (grade A) cover 19.29% of China. The stability grade is lowest in the Northeast, eastern Inner Mongolia, and northern Xinjiang. The winter-to-summer radiation ratio is below 0.28 in these areas, and they cover 20.03% of China. The other areas have moderate stability. In these areas, the northern parts generally have higher seasonal stability than the southern ones. The areas with grade B and grade C stabilities cover 30.47% and 29.82% of China, respectively.
Figure 8 shows the seasonal radiation difference between the TMY and MYA methods (i.e., Experiment A versus F). The difference is larger in spring and summer. The range of the absolute difference measured by the 0.99 quantile is 1.44% of the annual total in spring and 1.58% in summer. Autumn and winter show a relatively smaller difference, with a 0.99 quantile of 1.16% and 1.00%, respectively. The seasonal variations in the difference between the TMY and MYA methods reflect the activity of weather systems. Relatively active weather systems in summer increase the difference, whereas the difference is reduced in winter due to relatively stable weather conditions. The area with a notable seasonal difference coincides with the area with the abundance grade of C (Figure 3b), which is the middle and lower Yangtze River basins, the middle Yellow River basin, the Huaihe River basin, and northeast China. Northern China exhibits a slightly seasonal dependency. The difference in northeast China is notable in spring and summer but diminishes in winter. This seasonal variation in southern China is much weaker. The middle and lower Yangtze River basins are the areas with the most notable differences all year round. Unlike the difference in the annual total (Figure 5), the difference in the seasonal radiation is skewed around zero, and the skewness varies with season. MYA tends to have a slightly lower estimate in summer and a marginally higher estimate in spring than TMY. The median difference is —0.011% and 0.029% for summer and spring, respectively.
Figure 9 shows the difference in the stability index and grade between the TMY and MYA methods (i.e., Experiment A versus F). Consistent with the discussion above, the probability distribution function of the difference in the stability index is slightly skewed to the right, indicating that the MYA method tends to have a higher stability index than the TMY. The difference is more notable in southwestern China, including Yunnan, Sichuan, Guangdong, and Guangxi. The increase in the stability index is consistent with the lower summer and higher winter radiation, as shown in Figure 8. The difference in the seasonal stability grade is more notable compared with the annual total. A total of 10.5% of China has a different stability grade. Approximately 70% of these areas experience an upgrade, whereas the other 30% experience a downgrade.

3.3. Impacts of the Meteorological Variables

Figure 10 shows the difference between Experimnents I, J, and K to Experiment A. The difference delineates the impact of the meteorological variables on estimating the annual solar radiation. The impacts are marginally smaller than the difference between the TMY and MYA methods (Figure 5). The 0.99 quantiles of the absolute difference are 2.71%, 2.41%, and 2.57% of the annual total for wind speed, air temperature, and dew point, respectively. Wind speed generally has the most considerable impact among the three variables, with a median absolute difference of 1.85% of the annual total. The dew point has the second most considerable impact. The median absolute difference is 1.77% of the annual total. The air temperature makes the smallest difference with a median value of 1.68%. The three variables have similar patterns of impact. The impacts are more notable in northeast China and the middle Yangtze River basin, which have low solar energy resources (grades B and C as shown in Figure 3). The impacts of wind speed and dew point tend to have an opposite direction. Consideration of the wind speed slightly decreases the estimate (0.013% of the annual total in median), whereas consideration of the air temperature and dew point slightly increases the estimate (0.011% of the annual total in median).
Figure 11 is the same as Figure 10 but for the seasonal stability index. The impacts are all symmetric around zero for the three variables. Like the annual total as shown in Figure 10, the wind speed has the most considerable impact, the air temperature has the least significant effect, and the dew point lies in between. The range of the impacts measured by 0.99 quantiles of the absolute difference is similar for the three variables, which are 0.57 for wind speed, 0.054 for air temperature, and 0.054 for dew point. However, the median absolute difference is slightly larger for wind speed (0.035) than for temperature (0.032) and dew point (0.033). Unlike the annual total, the seasonal stability index’s changes are clustered only in the middle to lower Yangtze River basin and are negligible in the Northeast.

4. Conclusions

This study delineated the solar energy resources of mainland China using the TMY method and the CMFD dataset and the impacts from the records lengths in various reference periods. The areas with the abundance grades A, B, C, and D cover 28%, 42%, 29%, and 1% of the whole territory of China, respectively. The annual total solar radiation is most abundant (grade A) in the Tibetan Plateau, southern Xinjiang, and the Inner Mongolian Plateau. The solar energy resources are low (grace C or D) in the northeastern part of northeast China, the middle to lower Yangtze River basin. The other regions fall in between. The longer the data records, the more stable the assessment. The assessments become acceptably stable using data records that are equal to or longer than 30 years.
This study compared the TMY and MYA methods. Their differences in the annual total are symmetric around zero. The difference is mainly exhibited in Yunnan, Sichuan, Guangdong, Guangxi, and Shaanxi. The difference is nearly invariant with the data record length, hinting at the location-specific long-term weather characteristics. The differences in the seasonal stability index are more notable. The stability grade differs in approximately 10.5% of China. The region is mostly the same as that for the annual total. The difference in the seasonal stability is skewed. Among these regions with different stability grades, approximately 70% experience a downgrade from TMY, whereas the other 30% experience an upgrade. In these mentioned provinces, an assessment method that can consider weather characteristics (e.g., TMY) is preferred.
This study also revealed the impact of three meteorological variables (i.e., wind speed, air temperature, and dew point) on the TMY-based assessment. Wind speed generally has the most considerable impact, air temperature has the least significant effect, and dew point lies in between. The difference is notable in places with modest solar energy resources where the weather conditions are the most variable. The spatial pattern of the difference varies with the variables. All three variables exhibit different annual total and seasonal stability in the middle to lower Yangtze River basin; whereas, in the Northeast, the impact of air temperature is negligible.
The results suggest that weather conditions have notable impacts on the solar energy abundance and seasonal variations in southwest China. However, the region tends to have significant data uncertainty due to relatively limited in situ observations and complex topography. Future assessments based on satellite observations and high-resolution model simulations would be helpful to reduce uncertainty.

Author Contributions

Conceptualization, H.Z.; methodology, H.Z.; data curation, H.Z.; investigation, Z.S.; formal analysis, Z.S.; visualization, Z.S. and B.W.; Writing—original draft, Z.S., B.W., S.J., X.L. and S.H.; Writing—review & editing, H.Z.; supervision, H.Z.; project administration, Z.S.; funding acquisition, Z.S. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by the Science and Technology Project “The Research of Mechanism and Simulation on the Interaction between the Local Climate and Large-scale Renewable Energy Development” (Grant No. 4000-202155465A-0-0-00) of State Grid Corporation of China (SGCC).

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

The CMFD version 1.7 used in this study was provided by Dr. Jie He at the Institute of Tibetan Plateau Research, Chinese Academy of Sciences. Earlier versions of CMFD are downloadable at https://doi.org/10.11888/AtmosphericPhysics.tpe.249369.file (accessed on 14 November 2023). The solar radiation data from each experiment and the plotting scripts used in this study are available at https://github.com/hzheng88/paper-2024-china-solar-tmy-cmfd.

Acknowledgments

We sincerely thank Jie He at the Institute of Tibetan Plateau Research for his kindness in providing the latest CMFD.

Conflicts of Interest

Zongpeng Song, Bo Wang, Shuanglong Jin, Xiaolin Liu, and Shenbing Hua are employees of the China Electric Power Research Institute. The paper reflects the views of the scientists and not the company.

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Figure 1. Schematic diagram of the TMY generation procedure. The five three-hourly variables shown at the top are from CMFD.
Figure 1. Schematic diagram of the TMY generation procedure. The five three-hourly variables shown at the top are from CMFD.
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Figure 2. Study domain. Blue lines denote the Yangtze and Huai Rivers. Black lines denote the province boundaries.
Figure 2. Study domain. Blue lines denote the Yangtze and Huai Rivers. Black lines denote the province boundaries.
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Figure 3. China’s solar energy resources assessed using the TMY method for a thirty-year period (1991 to 2020). (a) annual global horizontal solar radiation, and (b) abundance grade of the solar energy resources. The definitions of the grades A, B, C, and D are described in Section 2.3.
Figure 3. China’s solar energy resources assessed using the TMY method for a thirty-year period (1991 to 2020). (a) annual global horizontal solar radiation, and (b) abundance grade of the solar energy resources. The definitions of the grades A, B, C, and D are described in Section 2.3.
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Figure 4. Relative changes in the solar radiation estimates using the reference periods of different lengths. The changes are relative to the thirty-year period from 1991 to 2020: (a) 10 years from 2011 to 2020; (b) 20 years from 2001 to 2020; (c) 40 years from 1981 to 2020; and (d) 50 years from 1971 to 2020.
Figure 4. Relative changes in the solar radiation estimates using the reference periods of different lengths. The changes are relative to the thirty-year period from 1991 to 2020: (a) 10 years from 2011 to 2020; (b) 20 years from 2001 to 2020; (c) 40 years from 1981 to 2020; and (d) 50 years from 1971 to 2020.
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Figure 5. Relative difference between the MYA and TMY methods in calculating annual solar radiation. The left panels present the spatial distribution, whereas the right panels present the probability distribution function (PDF).
Figure 5. Relative difference between the MYA and TMY methods in calculating annual solar radiation. The left panels present the spatial distribution, whereas the right panels present the probability distribution function (PDF).
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Figure 6. Seasonal radiation estimated with the TMY method for the thirty-year period (1991 to 2020). The values are fractions of the annual totals. (a) MAM for March, April, and May; (b) JJA for June, July, and August; (c) SON for September, October, and November; and (d) DJF for December, January, and February.
Figure 6. Seasonal radiation estimated with the TMY method for the thirty-year period (1991 to 2020). The values are fractions of the annual totals. (a) MAM for March, April, and May; (b) JJA for June, July, and August; (c) SON for September, October, and November; and (d) DJF for December, January, and February.
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Figure 7. Seasonal stability index and grade of the solar energy resource assessed using the TMY method for the thirty-year period (1991 to 2020). The seasonal stability index is defined as the ratio of the minimum monthly radiation to its maximum value. The stability grades A, B, C, and D are defined in Section 2.3.
Figure 7. Seasonal stability index and grade of the solar energy resource assessed using the TMY method for the thirty-year period (1991 to 2020). The seasonal stability index is defined as the ratio of the minimum monthly radiation to its maximum value. The stability grades A, B, C, and D are defined in Section 2.3.
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Figure 8. Difference between the MYA and TMY methods in calculating seasonal solar radiation for the thirty-year reference period (1991 to 2020). The values are presented as the percentage of the annual solar radiation estimated using the TMY method (Figure 3a).
Figure 8. Difference between the MYA and TMY methods in calculating seasonal solar radiation for the thirty-year reference period (1991 to 2020). The values are presented as the percentage of the annual solar radiation estimated using the TMY method (Figure 3a).
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Figure 9. Difference in the seasonal stability index and grade between the MYA and TMY methods: (a) Difference of the MYA method relative to TMY; (b) Difference in the seasonal stability grade of the MYA method relative to TMY. Red denotes an upgrade (up arrow), whereas blue denotes a downgrade (down arrow); (c) Probability distribution function (PDF) of the difference in the seasonal stability index.
Figure 9. Difference in the seasonal stability index and grade between the MYA and TMY methods: (a) Difference of the MYA method relative to TMY; (b) Difference in the seasonal stability grade of the MYA method relative to TMY. Red denotes an upgrade (up arrow), whereas blue denotes a downgrade (down arrow); (c) Probability distribution function (PDF) of the difference in the seasonal stability index.
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Figure 10. Sensitivity of annual solar radiation to the considered meteorological variables. The three rows present the impacts of wind speed, air temperature, and dew point, respectively. The right panels present the probability distribution function of the relative differences corresponding to the left panels.
Figure 10. Sensitivity of annual solar radiation to the considered meteorological variables. The three rows present the impacts of wind speed, air temperature, and dew point, respectively. The right panels present the probability distribution function of the relative differences corresponding to the left panels.
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Figure 11. Sensitivity of the seasonal stability index to the considered meteorological variables. The three rows present the impacts of wind speed, air temperature, and dew point, respectively. The right panels present the cumulative distribution function of the relative changes corresponding to the left panels. The lower and upper numbers in the right panels denote the CDFs of the area with negative and non-negative changes, respectively.
Figure 11. Sensitivity of the seasonal stability index to the considered meteorological variables. The three rows present the impacts of wind speed, air temperature, and dew point, respectively. The right panels present the cumulative distribution function of the relative changes corresponding to the left panels. The lower and upper numbers in the right panels denote the CDFs of the area with negative and non-negative changes, respectively.
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Table 1. Comparison between the MYA and TMY methods.
Table 1. Comparison between the MYA and TMY methods.
AspectMYATMY
Input dataUse solar radiation data only.Use solar radiation and multiple surface meteorological variables such as air temperature, wind speed, and dew point.
Calculation of annual solar radiationArithmetic average of the solar radiation data over multiple years.Arithmetic average of the solar radiation over a TMY. The TMY is generated using multiple meteorological variables.
Calculation of annual solar radiation cycle.Multi-year averaged annual cycleAnnual cycle of the TMY.
Consideration of extreme weather conditionsNo.Yes. Consider the climatology of extreme daily statistics such as maximum and minimum air temperature.
Table 2. Experimental settings.
Table 2. Experimental settings.
ExperimentMethodAveraging Weights 1Climatology
ATMY1/2, 1/12, 1/24, 1/24, 1/12, 1/24, 1/24, 1/12, & 1/121991–2020
BTMYThe same as A2011–2020
CTMYThe same as A2001–2020
DTMYThe same as A1981–2020
ETMYThe same as A1971–2020
FMYA-1991–2020
GTMYThe same as A2011–2020
HMYA-2011–2020
ITMY12/20, 2/20, 1/20, 1/20, 2/20, 1/20, 1/20, 0, & 01991–2020
JTMY12/20, 2/20, 1/20, 1/20, 0, 0, 0, 2/20, & 2/201991–2020
KTMY12/20, 0, 0, 0, 2/20, 1/20, 1/20, 2/20, & 2/201991–2020
1 The averaging weights of the Finkelstein–Schafer statistics for the surface downwelling solar irradiance, 2 m air temperature, daily maximum air temperature, daily minimum air temperature, dew point temperature, daily maximum dew point temperature, daily minimum dew point temperature, daily mean wind speed, and daily maximum wind speed, respectively.
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Song, Z.; Wang, B.; Zheng, H.; Jin, S.; Liu, X.; Hua, S. Gridded Assessment of Mainland China’s Solar Energy Resources Using the Typical Meteorological Year Method and China Meteorological Forcing Dataset. Atmosphere 2024, 15, 225. https://doi.org/10.3390/atmos15020225

AMA Style

Song Z, Wang B, Zheng H, Jin S, Liu X, Hua S. Gridded Assessment of Mainland China’s Solar Energy Resources Using the Typical Meteorological Year Method and China Meteorological Forcing Dataset. Atmosphere. 2024; 15(2):225. https://doi.org/10.3390/atmos15020225

Chicago/Turabian Style

Song, Zongpeng, Bo Wang, Hui Zheng, Shuanglong Jin, Xiaolin Liu, and Shenbing Hua. 2024. "Gridded Assessment of Mainland China’s Solar Energy Resources Using the Typical Meteorological Year Method and China Meteorological Forcing Dataset" Atmosphere 15, no. 2: 225. https://doi.org/10.3390/atmos15020225

APA Style

Song, Z., Wang, B., Zheng, H., Jin, S., Liu, X., & Hua, S. (2024). Gridded Assessment of Mainland China’s Solar Energy Resources Using the Typical Meteorological Year Method and China Meteorological Forcing Dataset. Atmosphere, 15(2), 225. https://doi.org/10.3390/atmos15020225

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