3.1. Sunphotometer Data
The ground data used to evaluate the VIIRS aerosol products in this study consists of CE318 sunphotometer (CE318) observations and retrievals. The CE318 instrument performs direct sun extinction measurements at eight wavelengths ranging from 340 to 1020 nm and sky radiance measurements at four wavelengths, i.e., 440, 675, 870, and 1020 nm. The AOD data were calculated from direct sun observations with an accuracy of 0.01 to 0.02 [
24,
25]. Refractive index, volume mean radius, volume concentration and single scattering albedo (SSA) retrieved from the CE318 sky measurements characterize the aerosol type. The uncertainties of refractive index are 30–50% for the imaginary part and 0.04 for the real part when AOD at 440 nm (AOD
440nm) > 0.4 and solar zenith angle > 50°, and the uncertainties increase for lower AODs [
26,
27]. SSA uncertainty is estimated to be less than 0.03 for AOD
440nm > 0.4 and the uncertainty increases for lower AODs [
26,
27]. Note that inversion data (size/optics) are sparse compared to direct sun observations of spectral AOD.
CE318 sunphotometer data (including the corresponding inversion products) over three sites in NCP region during the period of 2 May 2012–31 March 2014 were used. The location and description of the three CE318 sunphotometer sites are provided in
Table 1. These three sites can be considered as representative of urban (Beijing), suburban (XiangHe) and regional background (Xinglong) environments, respectively. Affected by Asian monsoons, the NCP region has a moderate continental climate with cold winters and hot summers. Heavy anthropogenic pollution from urbanization, industrial, and agricultural activities mixed with coarse dust particles (most occurring in spring) result in a rather complex nature of aerosol physical and optical properties in the NCP [
12]. Notably, the regional background station Xinglong is located at a mountain with the elevation of 970 m which is higher than the other two sites. However, even at this station, urban/industrial and dust aerosol could occur through aerosol regional transportation [
28] and secondary aerosol formation. Therefore, as will be shown in our analysis, the complex features of aerosol properties may help explain some of the uncertainties in satellite retrievals of AOD in this region.
Data at Beijing and XiangHe are downloaded from AERONET (
http://aeronet.gsfc.nasa.gov/) and the data at Xinglong are obtained from China Aerosol Remote Sensing Network (CARSNET) [
29]. AERONET level 1.5 inversion data (from sky-light measurements) are used since the level 2 inversion data are very less frequent and unsuitable for data statistics. At the same time, we used the conditions of AOD
440nm > 0.4 and solar zenith angle > 50° to constrain the data quality according to [
26,
27]. The AOD in these two networks are consistent with one another as the correlation coefficients are larger than 0.999 and have a 99.9% significance level [
29]. The CARSNET calibration and comparison with AERONET are described in detail in other references [
29,
30,
31].
It is noted that Beijing and XiangHe are part of AERONET stations, and their aerosol data during 2005 were used in the cluster analysis for the VIIRS_ML aerosol model assignment, but the Xinglong site was not used [
23]. Moreover, the retrieved aerosol properties in recent years may change from those used in 2005 and 2010 due to the rapid development in the past few years over the NCP region [
11,
12]. Therefore, using aerosol property data from more ground sites during recent years over this region can be used to help evaluate whether those past analyses from shorter periods (e.g., only one year) and fewer sites are still representative. Notably, none of these three sites were used in the analysis by Dubovik et al. [
27], which means they do not characterize typical aerosol properties of smoke, dust, and urban particles that have been adopted in the VIIRS_EDR algorithm. Thus, these three sites are better suited to evaluate the aerosol model type used in both the VIIRS_EDR and VIIRS_ML algorithms over the NCP region.
3.3. Methods for Aerosol Model Evaluation and Aerosol Properties Analysis
Due to constraints placed on the inversion of CE318 sky-radiance data (AOD440nm > 0.4; solar zenith angle > 50°, etc.), statistics for aerosol optical properties are sparse. To collocate aerosol optical properties from sunphotometer with aerosol models assumed by either VIIRS retrieval algorithm, we require different averaging domains. Here, we use daily-averaged aerosol optical properties retrieved from CE318 sky radiance measurements. Since the aerosol model types used for satellite AOD retrievals may vary spatially, we select only the model type assumed at the pixel that includes the site.
In the extraction of AOD from the VIIRS_EDR, those with quality QF < 1 retrievals are rejected (these with QF < 1 are not products and are mostly with cloud contamination and sunglint). Seasonal and total frequencies of each aerosol model type occurrence in the three sites are calculated to show the typical aerosol model types used in the VIIRS_EDR land algorithm over NCP sites.
The aerosol model type evaluation of VIIRS (VIIRS_EDR and VIIRS_ML) is based on the SSA comparisons between VIIRS and CE318. The SSA values at four wavelengths (440 nm, 670 nm, 870 nm and 1020 nm) of the five aerosol model types used in VIIRS_EDR can be obtained from Dubovik et al. [
27]. The values of SSA at 670 nm (SSA
670nm) are 0.98, 0.84, 0.93, 0.97 and 0.88 for dust, high absorption smoke, low absorption smoke, clean urban and polluted urban aerosol model, respectively. Thus, the SSA values at the NCP sites in the VIIRS_EDR retrival can be derived from the aerosol model type assumed in the VIIRS_EDR pixel that includes the site. The VIIRS_ML aerosol model type is assumed globally based on the cluster analysis of SSA
670nm derived from all AERONET inversions and it is fixed in each season for the NCP region (i.e., weakly absorbing fine model for Summer and Autumn: SSA
670nm ~ 0.95, moderately absorbing fine model for Spring and Winter: SSA
670nm ~ 0.90) [
22,
23], so it is unnecessary to extract the aerosol model from VIIRS_ML pixel-by-pixel. Thus, we do the seasonal comparison; that is, the seasonal mean SSA
670nm values of CE318 inversion are calculated and compared with the seasonal SSA
670nm values of the VIIRS_EDR and VIIRS_ML. Only the VIIRS SSAs with the AOD
550nm > 0.25 are used to meet the requirement of CE318 AOD
440nm > 0.4 [
23].
The SSA is also used to classify the aerosol type of the CE318 inversion, which is to evaluate the aerosol model type for each retrieval from the VIIRS algorithms. We firstly collocate the daily matchup data between the VIIRS_EDR and CE318 and between the VIIRS_ML and CE318. To evaluate the aerosol model type of VIIRS_EDR, the CE318 inversions are classified to the five aerosol types as the VIIRS_EDR. The CE318 inversion with Angstrom exponent < 0.6 and AOD at 1020 nm > 0.3 (according to Dubovik et al. [
27]) is classified as dust type. If not dust type, the CE318 inversion with SSA
670nm < 0.86 is the high absorption smoke, with 0.86 < SSA
670nm < 0.905 is polluted urban, with 0.905 < SSA
670nm < 0.95 is low absorption smoke, and with SSA
670nm > 0.95 is clean urban aerosol type. As for the evaluation of aerosol model type used in the VIIRS_ML, the CE318 inversions are classified to the four aerosol types as the VIIRS_ML. Use the same way to find out the CE318 data with coarse model (same as the dust). For the rest CE318 data, that with SSA
670nm < 0.875 is regarded as strong absorbing fine model, 0.875 < SSA
670nm < 0.925 is the moderately absorbing fine model, and SSA
670nm > 0.925 is the weakly absorbing fine model. The threshold values of the classification are based on the SSA values of the aerosol models used in the VIIRS algorithms. This method is actually using the aerosol size and scattering properties to classify the aerosol type, which has been studied by Giles et al. [
35]. After classifying the CE318 aerosol type, the comparisons of aerosol type between the VIIRS_EDR and CE318 and between the VIIRS_ML and CE318 are done to show the accuracy rate of aerosol model type used in the VIIRS_EDR and VIIRS_ML. If the VIIRS aerosol model type is same as that of CE318, the aerosol model type used in the VIIRS is deemed as accurate. The accuracy rate is defined as the ratio of the number of accurate to the number of all daily matchups. The accuracy rate reflects the applicability of aerosol model type used in the VIIRS algorithms.
We also conduct the SSA comparison of different modes (fine, coarse and bi-mode) between the VIIRS_EDR and CE318 retrieval. We compute the SSA for all aerosol modes at 440 nm in the VIIRS_EDR by inputting the aerosol parameters (refractive indices, size parameters and volume concentrations of each mode) into Mie scattering calculation [
36]. The reason for using 440 nm is that the aerosol model properties in the VIIRS_EDR algorithm are mostly referred at 440 nm [
6]. The input aerosol parameters of the VIIRS_EDR at each site are obtained by extracting the aerosol model type over the site pixel and calculated according to the
Table 2 in reference [
6]. Although SSA
440nm is available from CE318 inversion, for consistency we also use the Mie code to compute the SSA
440nm based on the aerosol optical properties inversed from CE318 sky radiances. We have compared the SSAs between the CE318 inversion and the Mie scattering calculation and the result shows that the bias of the two SSA values is very low (less than 0.01). That is because the CE318 inversion also uses Mie scattering calculation to obtain SSA. The resultant SSA
440nm of CE318 is compared with that of the VIIRS_EDR SSA
440nm. Since the CE318 sky-radiance inversion product is only reliable for AOD
440nm > 0.4, we also choose the aerosol properties of the VIIRS_EDR when AOD
550nm > 0.25 [
23].