Estimation of photosynthetically active radiation using solar radiation in the UV-visible spectral band

被引:18
|
作者
Zhian Sun [1 ]
Liang Hong [2 ]
Liu Jingmiao [3 ,4 ]
Shi Guoping [5 ]
机构
[1] Australian Bur Meteorol, Environm & Res Div, Melbourne, Vic 3001, Australia
[2] China Meteorol Adm, Meteorol Observat Ctr, Beijing 100081, Peoples R China
[3] China Meteorol Adm, Inst Atmospher Environm, Shenyang 110016, Liaoning, Peoples R China
[4] Chinese Acad Meteorol Sci, Beijing 100081, Peoples R China
[5] Nanjing Univ Informat Sci & Technol, Inst Geog & Remote Sensing, Nanjing, Jiangsu, Peoples R China
关键词
Photosynthetically active radiation; UV-visible band flux; Global horizontal irradiance; ALL-SKY CONDITIONS; TRANSMITTANCE MODEL; ASYMMETRY FACTOR; PARAMETERIZATION; ILLUMINANCE; IRRADIANCE; NETWORK; BEAM;
D O I
10.1016/j.solener.2017.06.007
中图分类号
TE [石油、天然气工业]; TK [能源与动力工程];
学科分类号
0807 ; 0820 ;
摘要
In this paper, we discuss a method using the UV-visible band flux to estimate photosynthetically active radiation (PAR). We use radiative transfer models to calculate the ratio of PAR to the UV-visible flux and confirm that this ratio is close to constant regardless of atmospheric conditions. The best ratio identified in this study is 0.8644. We further introduce a UV-visible band model and use it to calculate the PAR flux using observational datasets, mainly taken from the US SURFRAD network. The results are compared with the observations. It is seen that the PAR values determined using this method are in good agreement with observations. The relative mean biases (rMB) for both clear- and all-sky conditions evaluated for seven SURFRAD stations are -1.04% and -4.85%, respectively. The corresponding relative root mean square errors (rRMS) are 6.22% and 17.97%, respectively. (C) 2017 Elsevier Ltd. All rights reserved.
引用
收藏
页码:611 / 622
页数:12
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