Analysis of Atmospheric Turbidity in Clear Skies at Wuhan, Central China

被引:23
作者
Wang, Lunche [1 ]
Chen, Yisen [1 ]
Niu, Ying [1 ]
Ariel Salazar, German [2 ]
Gong, Wei [3 ]
机构
[1] China Univ Geosci, Sch Earth Sci, Dept Geog, Wuhan 430074, Hubei, Peoples R China
[2] Salta Natl Univ, Sch Exact Sci, Dept Phys, A4408FVY, Salta, Argentina
[3] Wuhan Univ, State Key Lab Informat Engn Surveying Mapping & R, Wuhan 430079, Hubei, Peoples R China
基金
中国国家自然科学基金;
关键词
direct solar radiation; Angstrom turbidity coefficient; Linke turbidity factor; Central China; SOLAR-RADIATION; COEFFICIENT BETA; OPTICAL-PROPERTIES; VALUES; IRRADIANCE; PARAMETERS; ATHENS;
D O I
10.1007/s12583-017-0756-2
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The Angstrom turbidity coefficient (beta) and Linke turbidity factor (T-L) are used to study the atmospheric conditions in Wuhan, Central China, using measured direct solar radiation during 2010-2011 in this study. The results show that annual mean beta values generally increase from 0.28 in the morning to 0.35 at noon, and then decrease to 0.1 in the late afternoon during the day; annual mean T-L generally varies from 3 to 7 in Central China. Both turbidity coefficients have maximum values in spring and summer, while minimum values are observed in winter months. It also reveals that beta values show preponderance (52.8%) between 0.15 and 0.35, 78.1% of T-L values are between 3.3 and 7.7, which can be compared with other sites around the world. Relationship between turbidity coefficients and main meteorological parameters (humidity, temperature and wind direction) have been further investigated, it is discovered that the local aerosol concentrations, dust events in northern China and Southwest Monsoon from the Indian Ocean influences the beta values in the study area.
引用
收藏
页码:729 / 738
页数:10
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