Luminous efficacies are determined at Madrid for North, South, East, West f
acing surfaces in two ways: by taking into account all the global illuminan
ce and irradiance values available, and by considering data for each of thr
ee sky categories as defined from values of the sky clearness index epsilon
' and the sky brighteness index Delta. Both methods are compared, and for
epsilon ' < 1.23 (overcast skies) the second method is found to be more acc
uarate than the first. (C) 1999 Elsevier Science Ltd. All rights reserved.