Evaluation of solar spectral irradiance distribution using an index from a limited range of the solar spectrum

• Published in: Current applied physics Vol. 14; no. 5; pp. 731 - 737
• Main Authors: Kataoka, Naoya, Yoshida, Shota, Ueno, Seiya, Minemoto, Takashi
• Format: Journal Article
• Language: English
• Published: Elsevier B.V 01.05.2014; 한국물리학회
• Subjects: Average photon energy; Energy distribution; Irradiance; Mathematical analysis; Photons; Photovoltaic cells; Photovoltaic module; Solar cells; Solar spectrum; Spectra; Spectral irradiance distribution; Wavelengths; 물리학; Solar spectrum; Average photon energy; Photovoltaic module; Spectral irradiance distribution
• ISSN: 1567-1739; 1878-1675
• DOI: 10.1016/j.cap.2014.03.004

The output energy of photovoltaic (PV) modules under outdoor conditions is greatly influenced by the spectral irradiance distribution of the solar spectrum. To analyze this effect on PV modules, the spectral irradiance distribution, which is one-dimensional data, has to be represented by a zero-dimensional index. The average photon energy (APE) is an index for spectral irradiance distributions, which represents the average energy per photon in a spectrum. We have previously analyzed the uniqueness of the shape of the solar spectrum in the wavelength range of 350–1050 nm, and one corresponding value of APE showed a specific shape of spectral irradiance distribution. In this study, new indexes were calculated for a limited wavelength range of 350–750 nm and multiple bands of 450–500 nm and 800–850 nm of the solar spectrum for easy measurement and calculation. The result shows the uniqueness of new indexes to the shape of measured solar spectrum and the standard deviations were found to be quite small. This indicates that the new indexes are reasonable for representing the spectral irradiance distribution and its effect on PV performance. •Solar spectra were indexed by existing and new indexes.•New index was obtained from only two bands of 50 nm of solar spectrum.•New index has the uniqueness to spectral distribution of 350–1050 nm.•One value of the new index represents one specific solar spectrum.•New index can replace to the existing index.