In this study, the tropospheric NO2 vertical column density (VCD) over an urban site in Guangzhou megacity in China is investigated by means of MAX-DOAS measurements during a campaign from late March 2015 to mid-March 2016. A MAX-DOAS system was deployed at the Guangzhou Institute of Geochemistry of the Chinese Academy of Sciences and operated there for about 1 year, during the spring and summer months. The tropospheric NO2 VCDs retrieved by the MAX-DOAS are presented and compared with space-borne observations from GOME-2/MetOp-A, GOME-2/MetOp-B and OMI/Aura satellite sensors. The comparisons reveal good agreement between satellite and MAX-DOAS observations over Guangzhou, with correlation coefficients ranging between 0.795 for GOME-2B and 0.996 for OMI. However, the tropospheric NO2 loadings are underestimated by the satellite sensors on average by 25.1, 10.3 and 5.7 %, respectively, for OMI, GOME-2A and GOME-2B. Our results indicate that GOME-2B retrievals are closer to those of the MAX-DOAS instrument due to the lower tropospheric NO2 concentrations during the days with valid GOME-2B observations. In addition, the effect of the main coincidence criteria is investigated, namely the cloud fraction (CF), the distance (d) between the satellite pixel center and the ground-based measurement site, as well as the time period within which the MAX-DOAS data are averaged around the satellite overpass time. The effect of CF and time window criteria is more profound on the selection of OMI overpass data, probably due to its smaller pixel size. The available data pairs are reduced to half and about one-third for CF <= 0.3 and CF <= 0.2, respectively, while, compared to larger CF thresholds, the correlation coefficient is improved to 0.996 from about 0.86, the slope value is very close to unity (similar to 0.98) and the mean satellite underestimation is reduced to about half (from similar to 7 to similar to 3.5 x 10(15) molecules cm(-2)). On the other hand, the distance criterion affects mostly GOME-2B data selection, because GOME-2B pixels are quite evenly distributed among the different radii used in the sensitivity test. More specifically, the number of collocations is notably reduced when stricter radius limits are applied, the r value is improved from 0.795 (d <= 50 km) to 0.953 (d <= 20 km), and the absolute mean bias decreases about 6 times for d <= 30 km compared to the reference case (d <= 50 km).
机构:
Key Laboratory for Aerosol-Cloud-Precipitation of China Meteorological Administration, Nanjing,210044, China
School of Atmospheric Physics, Nanjing University of Information Science & Technology, Nanjing,210044, ChinaKey Laboratory for Aerosol-Cloud-Precipitation of China Meteorological Administration, Nanjing,210044, China
Yu, Qing-Yuan
Yin, Yan
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Key Laboratory for Aerosol-Cloud-Precipitation of China Meteorological Administration, Nanjing,210044, China
School of Atmospheric Physics, Nanjing University of Information Science & Technology, Nanjing,210044, ChinaKey Laboratory for Aerosol-Cloud-Precipitation of China Meteorological Administration, Nanjing,210044, China
Yin, Yan
Zhang, Xin
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Key Laboratory for Aerosol-Cloud-Precipitation of China Meteorological Administration, Nanjing,210044, China
School of Atmospheric Physics, Nanjing University of Information Science & Technology, Nanjing,210044, ChinaKey Laboratory for Aerosol-Cloud-Precipitation of China Meteorological Administration, Nanjing,210044, China
机构:
Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Hendrick, F.
Muller, J-F
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Muller, J-F
Clemer, K.
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Clemer, K.
Wang, P.
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Chinese Acad Sci, Inst Atmospher Phys, Beijing, Peoples R ChinaBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Wang, P.
De Maziere, M.
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
De Maziere, M.
Fayt, C.
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Fayt, C.
Gielen, C.
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Gielen, C.
Hermans, C.
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Hermans, C.
Ma, J. Z.
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Chinese Acad Meteorol Sci, Beijing, Peoples R ChinaBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Ma, J. Z.
Pinardi, G.
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Pinardi, G.
Stavrakou, T.
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Stavrakou, T.
Vlemmix, T.
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Belgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Delft Univ Technol TU Delft, Delft, NetherlandsBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium
Vlemmix, T.
Van Roozendael, M.
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Belgian Inst Space Aeron BIRA IASB, Brussels, BelgiumBelgian Inst Space Aeron BIRA IASB, Brussels, Belgium