Two different procedures are explored in the present work to estimate the z
enith luminance at the International Daylight Measurement Program station i
n Madrid, when all the data available are used independently of the sky typ
e. On the basis of the results obtained, correlations for the seasonal depe
ndence of the zenith luminance on solar elevation are reported. However, it
is observed that polynomials obtained for different ranges of the luminous
clearness index, the ratio of global to extraterrestrial illuminance, can
predict the zenith luminance with a more reasonable accuracy. The results s
how that the luminous clearness index is an important parameter for zenith
luminance characterization, to be used when global illuminance values on ho
rizontal surfaces are available, but diffuse illuminance is not measured (C
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