This paper presents a comparison between some new models for representing sky luminance, as proposed by Kittler, Darula and Perez, and some typical skies recorded in Sydney, Australia. The results of this study show that these new models are most probably better suited to model skies that are clear or fully overcast as compared with the CIE standard sky models. Skies that have partial cloud coverage are typically more complex than can be modelled using standard models. In such cases special local models would have to be devised.
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References
1.
Commission Internationale de l'EclairageSpatial distribution of daylight: luminance distribution of various reference skies Technical Report CIE 110 (Vienna: CIE Central Bureau) (1993)
2.
Commission Internationale de l'EclairageStandarization of luminance distributions on clear skies Publication 22 (Paris: CIE Central Bureau) (1973)
3.
Commission Internationale de L'EclairageStandard overcast and clear sky 3rd Draft Div 3 (Vienna : CIE) (1990)
4.
Ruck N., Hayman S. and Julian W.The development and verification of sky models which represent the predominant skies in Australia for the predictions of daylight in buildings ( University of New South Wales) (1990 )
5.
Hayman S.The daylight climate of Sydney (PhD thesis, University of Sydney) (1997)
6.
Harrison A.Directional luminance versus cloud cover and solar positionSolar Energy4613-20 (1991)
7.
Nakamura H., Oki M. and Hayashi Y.Luminance distribution of intermediate sky J. Light VisualEnviron. 9(1) 6-13 (1985)
8.
Perez R., Seals R. and MichalskyJ An all-weather model for sky luminance distributionSolar Energy50(3) 235-245 (1991)
9.
Kittler R., Darula S. and Perez R.A set of standard skies (Bratislava: Institute of Construction and Architecture, Slovak Academy of Sciences) (1998)
10.
Kittler R., Darula S. and Perez R.A new generation of standard skiesProceedings Lux Europa (Antsterdam: Association of Lighting Societies in Europe) pp 359-373 (1997)
11.
Tregenza P.Subdivision of the sky hemisphere for luminance measurementsLighting Res. Technol.1913—14( 1987)
12.
Roy G.G., Hayman S. and Julian W.Sky modelling from digital imagery ARC Project No. A89530177 Final Report (University of Sydney and Murdoch University) (1998) URL: http://eng.murdoch.edu.au/FTPsite/daylighting.html
13.
Roy G.G., Ruck N. and Winkelmann F.New modelling technologies for sky luminanceProceedings CIE 23rd Session, New Delhi pp 327-328 (1995)
14.
Roy G.G., Ruck N., Reid G., Winkelmann F.C. and Julian W.The development of modeling strategies for whole sky spectrums under real conditions for international use ARC Project Report A89131897 ( School of Engineering, Murdoch University) (Sept 1995) URL: http://eng.murdoch.edu.au/FTPsite/daylighting.html
15.
Roy G.G., Ruck N., Reid G. and Julian W.Sky luminance: standard digital form for modellingLighting Res. Technol.27(3) 161-167 (1995)
16.
Reid G.Interpolation and contouring of discontinuous discrete data (MSc thesis, University of Western Australia) (1997)
17.
Kocifaj M.ModelSky (Bratislava: Institute of Construction and Architecture) (1998)
Perez R., Seals R. Michalsky J and Ineichen P Geostatistical properties and modeling of random cloud patterns for real skiesSolar Energy51(1) 7-18(1993)
20.
Ineichen P. , Molineaux B. and Perez R.Sky luminance data validation; comparison of 7 models with 4 data banks. Solar Energy52(4) 337-34 (1994)