透射率
红外窗口
照度
光合有效辐射
辐射
漫射天空辐射
光学
辐照度
摩尔吸收率
太阳辐照度
环境科学
红外线的
光谱带
遥感
物理
水蒸气
天空
材料科学
大气科学
气象学
散射
化学
生物化学
地质学
光合作用
标识
DOI:10.1016/0038-092x(89)90113-8
摘要
A two-band radiation modelling technique is proposed for the clear sky case. The solar spectrum is divided into a UV/Visible band (0.29–0.7 μm) and an infra-red band (0.7–2.7 μm). In each band, the transmittance of each extinction layer (ozone, water vapor, mixed gases, molecules and aerosols) is parameterized using preliminary integrations of state-of-the-art spectral transmittance functions. The beam and diffuse radiation components are obtained as functions of these layer transmittances. The photosynthetically active radiation (0.4–0.7 μm) and illuminance (0.39–0.76 μm) components may be easily derived from the UV/Visible band irradiances. In the case of typical atmospheric conditions, the model predictions are generally in good agreement with results from three accepted rigorous spectral codes. The effect of changing the solar elevation, the Angström turbidity coefficient and the site altitude on the beam, diffuse and global components (or their ratio) is further discussed.
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