A combination of a photodiode with a nonimaging light concentrator is
developed to perform measurements of the direct solar radiation compon
ent. A prototype composed of low price elements is taken as a starting
point to discuss the problems which must be faced when calibrating su
ch sensors. By this the influence of the angle of incidence and spectr
al distribution (caused by different air mass or varying degree of cle
arness) of the incident radiation on the behavior of the system is stu
died. The readings are compared to the calculated (global minus diffus
e) readings obtained from two standard star pyranometers. Finally the
possibilities for increasing the accuracy of the sensor element and fo
r applying the device are discussed. (C) 1998 Elsevier Science Ltd. Al
l rights reserved.