A two-band model for the calculation of clear sky solar irradiance, illuminance, and photosynthetically active radiation at the earth's surface

Journal Article · Sat Dec 31 23:00:00 EST 1988 · Solar Energy; (USA)

DOI:https://doi.org/10.1016/0038-092X(89)90113-8· OSTI ID:5062408

Gueymard, C ^[1]

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1. Serres Bio-Solaire Inc., Ham-Nord (Canada)

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 {mu}m) and an infra-red band (0.7-2.7 {mu}m). 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 {mu}m) and illuminance (0.39-0.76 {mu}m) 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 Angstrom turbidity coefficient and the site altitude on the beam, diffuse and global components (or their ratio) is further discussed.

• OSTI ID: 5062408
• Journal Information: Solar Energy; (USA), Journal Name: Solar Energy; (USA) Vol. 43:5; ISSN SRENA; ISSN 0038-092X
• Country of Publication: United States
• Language: English

Related Subjects

14 SOLAR ENERGY
140100* -- Solar Energy-- Resources & Availability
ALTITUDE
CALCULATION METHODS
CHEMICAL REACTIONS
DIFFUSE SOLAR RADIATION
DIRECT SOLAR RADIATION
ELECTROMAGNETIC RADIATION
MATHEMATICAL MODELS
PHOTOCHEMICAL REACTIONS
PHOTOSYNTHESIS
RADIATIONS
SOLAR FLUX
SOLAR RADIATION
STELLAR RADIATION
SYNTHESIS
TURBIDITY
ULTRAVIOLET RADIATION
VISIBLE RADIATION