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Sky luminance distribution in the North of Iberian Peninsula during winter
Authors:JL Torres  M de Blas  A García  A Gracia  A de Francisco
Institution:1. Department of Projects and Rural Engineering, Public University of Navarre, Edificio Los Olivos, 31006 Pamplona, Spain;2. Department of Forestry Engineering, Polytechnic University of Madrid, Ciudad Universitaria, 28040 Madrid, Spain;1. Department of Electrical Engineering, Techno India, Salt Lake, Kolkata 700091, West Bengal, India;2. Department of Electrical Engineering, Jadavpur University, Kolkata 700032, West Bengal, India;1. Department of Electrical and Electronics Engineering, Dokuz Eylul University, Buca 35160, Izmir, Turkey;2. Department of Electrical and Electronics Engineering, Ege University, Bornova 35100, Izmir, Turkey;3. Department of Electrical and Computer Engineering, Kumamoto University, 860-8555 Kumamoto, Japan;1. Department of Electronics and Electrical Engineering, Shiraz University of Technology, Shiraz, Iran;2. Australian Power Quality and Reliability Centre, School of Electrical, Computer and Telecommunications Engineering, University of Wollongong, Australia
Abstract:This work is based on the study of outdoor daylight conditions during the winter period in Pamplona (the Iberian Peninsula). The 15 standard sky types proposed by the Commission Internationale de l’Eclairage (CIE) are used. The selected sky type in each moment is the one exhibiting the lowest root mean standard deviation (RMSD) when the theoretical and experimental luminance distributions in the sky hemisphere are compared. The selection was derived from luminance distribution data from 145 patches of the sky hemisphere and registered every 10 min from October to March from 2007 and 2008.The most frequent sky type observed in winter in Pamplona is V.5 (cloudless polluted with a broad solar corona), with a frequency of occurrence of 21%. Notwithstanding, the group of overcast skies exhibits a slightly higher frequency (40%) than the clear skies (37%). Seven out of the 15 standard sky types, i.e.V.5, I.1, III.4, II.1, IV.4, II.2 and III.3, are practically 80% of those under study. In order to provide a possible application in daylight climates studies, the frequency of occurrence of the 15 sky types is included in eleven intervals of solar elevation on the threshold corresponding to the time period and the location considered.
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