| | Optical Society of San Diego |
 | | I developed a custom computer program to isolate skyglow pixel values by removing CCD noise and star pixels from the images and to compute the average intensity of the skyglow pixels, from 0 to 765, for each image. |
 | | The amount of skyglow at 45 to 60-degree angles of observation averaged up to 220% more than zenith skyglow values for the same distance and up to 87% average increase at 120 to 135 degrees. |
 | | Conclusions: The amount of skyglow (S) decreased inversely with the distance (d) from the urban center, as approximated by the equation: S = 2.4 X 10^2 X d^-1.9 per one degree of sky, with significantly greater amounts of skyglow for non-zenith angles of observation both towards and away from the urban center. |
| www.osa.org /localsections/ossd/EdOutreach/Gsdsef/gsdsef2004/gsdsef2004_jake.htm (710 words) |