- Rayleigh (unit)
The rayleigh is a unit of
luminous flux used to measureair glow (auroras, for example). It was first proposed in 1956 by D. M. Hunten, noredlink|Franklin E. Roach, and J. W. Chamberlain. It is named forRobert John Strutt, 4th Baron Rayleigh (1875 –1947 ).Fact|date=November 2007 Its symbol is R (also used for theröntgen , an unrelated unit). The SI prefixes are used with the rayleigh.One rayleigh (1 R) is defined as a column emission rate of 1010
photon s persquare metre per column persecond . Note that rayleigh is an apparent emission rate, as no allowances have been made for scattering or absorption. The night sky has a luminous intensity of about 250 R, while auroras can reach values of 1000 kR.The relationship between radiance, "L", (in units of photons per square metre per second per
steradian ) and "I" (in units of rayleighs) is simply:"L" = "I" × frac|1010|4π
References
* D. M. Hunten, Franklin E. Roach, and J. W. Chamberlain (1956), A photometric unit for the airglow and aurora, Journal of Atmospheric and Terrestrial Physics (GB), Volume 8, pp 345-346
Wikimedia Foundation. 2010.