Skyglow: a retrieval of the approximate radiant intensity function of ground-based light sources

被引:13
作者
Kocifaj, M. [1 ,2 ]
Solano Lamphar, H. A. [2 ,3 ]
机构
[1] Comenius Univ, Dept Expt Phys, Fac Math Phys & Informat, Bratislava 84248, Slovakia
[2] Slovak Acad Sci, ICA, Bratislava 84503, Slovakia
[3] Inst Invest Lumin, Los Mochis, Sinaloa, Mexico
关键词
radiative transfer; atmospheric effects; light pollution; methods: observational; site testing; NIGHT-SKY BRIGHTNESS; AEROSOL OPTICAL-THICKNESS; MULTIPLE-SCATTERING; PLANETARY-ATMOSPHERES; POLARIZED-LIGHT; POLLUTION; CLOUDY; MODEL; OBSERVATORIES; ILLUMINATION;
D O I
10.1093/mnras/stu180
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Our research has been conducted with the specific objective to identify an efficient theoretical technique for retrieval of the emission pattern of ground-based light sources in order to determine the optimum values of the scaling parameters of the Garstang function. In particular, the input data involve the zenith luminance or radiance with horizontal illuminance or irradiance. Theoretical ratios of zenith luminance L-V(0) to horizontal illuminance D-V are calculated for a set of distances d that separate a hypothetical observer from the light source (a city or town). This approach is advantageous because inexpensive traditional equipment can be used to obtain the mean values of the Garstang parameters. Furthermore, it can also be applied to other parametrizable emission functions and to any measuring site, even one with a masked horizon.
引用
收藏
页码:3405 / 3413
页数:9
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