作者:Wang, LC (Wang, Lunche); Salazar, GA (Salazar, German Ariel); Gong, W (Gong, Wei); Peng, SM (Peng, Simao); Zou, L (Zou, Ling); Lin, AW (Lin, Aiwen)
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摘要:The accurate determination of the atmospheric turbidity is of great importance for atmospheric environment, solar energy applications and climate change studies. Daily values of horizontal direct, diffuse and global solar radiation at Wuhan, Central China during 1961-2010 are used for estimating the monthly mean Angstrom turbidity coefficient beta. The YHM and YHM2 (Yang hybrid models) are first used to estimate the direct and diffuse components considering the transmittances of ozone, water vapor, gas mixture, aerosol and Rayleigh effect in the radiative transfer processes. An IMW (improved model for Wuhan) is also proposed by combining the format of YHM model with the corrected spectral terms of YHM2 model. Then, the beta value can be estimated by varying the estimated direct irradiation until it matches the observation. The model performance is analyzed and compared and further validated by measured values using Sun photometer CE318. It is shown that the IMW model presents more accurate estimates than YHM and YHM2 ones; it is therefore a useful tool for studying the variability and evolution of atmospheric turbidity in other places around the world. (C) 2014 Elsevier Ltd. All rights reserved.
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地址:[Wang, Lunche; Gong, Wei] Wuhan Univ, State Key Lab Informat Engn Surveying Mapping & R, Wuhan 430079, Hubei Province, Peoples R China.
[Wang, Lunche; Gong, Wei] Collaborat Innovat Ctr Geospatial Technol, Wuhan 430079, Peoples R China.
[Salazar, German Ariel] Natl Univ Salta, Dept Phys, Sch Exact Sci, RA-4408 Fvy Salta Capital, Argentina.
[Peng, Simao; Zou, Ling; Lin, Aiwen] Wuhan Univ, Sch Resource & Environm Sci, Wuhan 430079, Hubei Province, Peoples R China.
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通讯作者地址:Wang, LC (通讯作者),Wuhan Univ, State Key Lab Informat Engn Surveying Mapping & R, Wuhan 430079, Hubei Province, Peoples R China.
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