Issues concerning atmospheric turbidity indices

被引:22
作者
Eltbaakh, Yousef A. [1 ]
Ruslan, M. H. [2 ]
Alghoul, M. A. [2 ]
Othman, M. Y. [2 ]
Sopian, K. [2 ]
机构
[1] Univ Kebangsaan Malaysia, Dept Phys, Bangi 43600, Selangor, Malaysia
[2] Univ Kebangsaan Malaysia, Solar Energy Res Inst, Bangi 43600, Selangor, Malaysia
关键词
Solar attenuation; Atmospheric aerosol; Atmospheric turbidity indices; AEROSOL OPTICAL-THICKNESS; SOLAR-RADIATION; LINKE; COEFFICIENT; ATHENS; MODEL; PARAMETERS; RETRIEVAL; VALUES;
D O I
10.1016/j.rser.2012.05.034
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
Knowledge of atmospheric turbidity coefficients is very important in meteorology, climatology, atmospheric pollution monitoring, and in the prediction of solar energy availability under cloudless skies. This paper provides a thorough review on a number of atmospheric turbidity indices and on the several methods that have been developed in the past few decades. The Lambert-Bouguer-Beer law is the basic relationship underlying the derivation of various turbidity indices. Turbidity can be referred to as monochromatic (narrow band) wavelengths, broadband wavelengths, and the total spectrum. Narrow band turbidity is measured using sun photometers, while the other two turbidities are measured using pyrheliometers with broadband pass filters. The Angstrom's turbidity coefficients and the Linke's turbidity factor are among the most frequently used atmospheric turbidity coefficients. (C) 2012 Elsevier Ltd. All rights reserved.
引用
收藏
页码:6285 / 6294
页数:10
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