Amid daytime the measure of enlightenment and spectraldistribution of light (shade) arriving at a scene depends onthe time of day and environmental conditions. The colorspectrum of the light arriving at the scene is imperative ifcolor CCTV is being utilized. Immediate daylight produces thehighest-contrast scene, permitting greatest identificationof objects. On a shady or cloudy day, less light is receivedby the articles in the scene bringing about less differentiation. Toproduce an ideal cam picture under the wide variationin light levels (daytime to evening), an automaticiriscamera framework is needed. Table 2-1 demonstrates the lightlevels for open air enlightenment under brilliant sun, partialclouds, and cloudy day down to cloudy night.scene light is measured in foot candles (Fc)and can change over a scope of 10,000 to 1 (or more). Thisexceeds the element working scope of most cam sensorsfor creating a decent quality feature picture. After thesun has gone beneath the skyline and if the moon is overhead,reflected daylight from the moon enlightens the scene and may be identified by a touchy monochromecamera. Recognition of data in a scene under thiscondition obliges an extremely touchy cam since there isvery minimal light reflected into the cam lens from thescene. As an amazing, when the moon is not overheador is darkened by shadiness, the main light gotten isambient light from: (1) neighborhood man-made lighting sources,(2) night-shine brought about by inaccessible ground lighting reflectingoff particulate (contamination), mists, and mist concentrates in thelower air, and (3) immediate light created by starlight.this is the most serious lighting condition and requireseither: (1) ICCD, (2) monochrome cam with IR Ledillumination, or (3) warm IR cam. Table summarizesthe light levels happening under sunlight and theselll conditions and the working scopes of normal cameras.the equal metric measure of light level (lux)compared with the foot candle (Fc) is given. One Fc isequivalent to roughly 9 lux.