The rayleigh is a unit of luminous flux used to measure air glow (auroras, for example). It was first proposed in 1956 by D. M. Hunten, Franklin E. Roach, and J. W. Chamberlain. It is named for Robert John Strutt, 4th Baron Rayleigh (1875 – 1947). Its symbol is R (also used for the röntgen, an unrelated unit). The SI prefixes are used with the rayleigh. One rayleigh (1 R) is defined as a column emission rate of 1010 photons per square metre per column per second. 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 x 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
