Stilb (unit) explained

The stilb (sb) is the CGS unit of luminance for objects that are not self-luminous. It is equal to one candela per square centimeter or 10⁴ nits (candelas per square meter). The name was coined by the French physicist André Blondel around 1920.^[1] It comes from the Greek word Greek, Ancient (to 1453);: stilbein, meaning 'to glitter'.

It was in common use in Europe up to World War I. In North America self-explanatory terms such as candle per square inch and candle per square meter were more common.^[2] The unit has since largely been replaced by the SI unit: candela per square meter. The current national standard for SI in the United States discourages the use of the stilb.^[3]

See also

• Scotopic stilb

Further reading

• Stilb at A Dictionary of Units of Measurement, Russ Rowlett and the University of North Carolina at Chapel Hill. Accessed June 2008.
• Stilb at Sizes.com. Accessed June 2008.

Notes and References

1. Parry Moon. "System of photometer concepts", in the Journal of the Optical Society of America, volume 32, number 6 (June 1942). – Page 355: "The lumen was proposed by Blondel in 1894 and is now universally accepted. The names, phot and stilb were likewise coined by Blondel (1921) and are in general use on the Continent."
2. American Standard Definitions of Electrical Terms, New York: American Institute of Electrical Engineers, 1941.
3. IEEE/ASTM SI 10-2002. American National Standard for Use of the International System of Units (SI): The Modern Metric System. New York: IEEE, 30 December 2002. See Section 3.3.3.