The paper introduces a method which allows the consideration of the curvature and stratification of the atmosphere when determining relative optical air mass. Formulae for relative optical air mass determination for places at sea level, at higher altitudes and for cloud formations are presented. These formulae were derived to promote further sky model development.
Get full access to this article
View all access options for this article.
References
1.
Fesenkov V.The brightness of the clear diurnal sky considering sphericalEarth Trans. USSR Academy of Scien. 101(5) 845-847 (1955)
2.
Bodmann H.W. , Burger W. and Liebelt ChPhotometrisches und radiometrisches Modell des trüben HimmelsProc. 19th Session CIE, Kyoto P-79-73 451-454 (1979)
3.
Nagata T.Luminance distribution of clear sky and resultant horizontal illuminanceJ. Light Vis. Env.7(1) 23-27 (1983)
4.
Kittler R. and Pulpitlová J.Basis of the utilization of daylight (Bratislava : VEDA Publishers) (1988)
5.
Baur F.Linke's meteorologisches Taschenbuch B. II, (Tabl. 91) ( Leipzig: Akademische Verlagsgesellschaft Geest and Portig K-G) (1953)
6.
Kittler R. and Mikler J.Basis of the utilization of solar radiation (Bratislava : VEDA Publishers) (1986)
7.
Machotkin L.G.Equivalent to Bemporad's air mass Trudy Glav , Geofiz. Observ.10015-16 (1960)
8.
Foitzik L. and Hinzpeter H.Sonnenstrahlung und Lufttrübung (Leipzig: Akademische Verlagsgesellschaft Geest and Portig K-G) ( 1958)