The Precision Solar Spectroradiometer (PSR) for direct solar irradiance measurements

被引:14
作者
Grobner, Julian [1 ]
Kouremeti, Natalia [1 ]
机构
[1] World Radiat Ctr, Phys Meteorol Observatorium Davos, Dorfstr 33, CH-7260 Davos, Switzerland
关键词
Solar irradiance measurements; Spectroradiometer; Calibration; Characterisation; Instrument intercomparison; Aerosol optical depth; STRAY LIGHT CORRECTION; SPECTRAL IRRADIANCE; ARRAY SPECTRORADIOMETERS; PERFORMANCE;
D O I
10.1016/j.solener.2019.04.060
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
A precision solar spectroradiometer (PSR) has been designed for high precision and accurate measurements of direct normal spectral solar irradiance in the wavelength range 300-1000 nm. Each PSR is radiometrically characterised and calibrated in the optical laboratory of PMOD/WRC. The calibration is traceable to SI through the primary spectral irradiance standard of the Physikalisch-Technische Bundesansalt (PTB), in Braunschweig, Germany. The expanded relative uncertainty for spectral solar irradiance measurements in the 350-1000 nm range is between 1.7% and 2.0%, with larger uncertainties below 400 nm which are mainly caused by the low signal levels and the uncertainties due to the straylight correction. A solar extraterrestrial spectrum was retrieved from solar measurements using the Langley-technique at a high altitude observatory and was found to be in excellent agreement with a literature solar spectrum (mean ratio 0.998 +/- 0.019). On two clear sky days solar measurements from 3 PSR and one independently calibrated spectroradiometer deployed during the International Pyrheliometer Comparison agreed to within their combined expanded uncertainties of 3%. Aerosol optical depth retrieved from the same solar measurements of the three PSR showed median differences with respect to the World reference for AOD between - 0.010 and + 0.014 at the center wavelengths 368 nm, 412 run, 500 nm, and 862 nm. The instrument has a second auxiliary port for connecting different entrance optics for near coincident measurements such as global solar irradiance.
引用
收藏
页码:199 / 210
页数:12
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