Overview
The skot to measure the dark luminance () was introduced in 1940 by the (, LiTG) out of a necessity to describe the luminance of self-luminous objects, which differed so much from that of other objects that it was impractical to describe it using commonly used luminance values. Conversion factors for so called "scotopic stilb" () depend on the spectral distribution of the light and were therefore redefined in 1948 by the International Commission on Illumination (, IBK) for a specific color temperature of 2042 K or 2046 K, the temperature of solidification ofUnit conversions
See also
* Nox (unit) to measure the dark illuminance () * Purkinje effect * Photometry (optics) * Scotopic lux * Scotopic visionReferences
Further reading
* * * * (2 pages) * * (8 pages) {{SI light units Units of luminance Centimetre–gram–second system of units