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The rayleigh is a unit of photon flux, used to measure faint light emitted in the sky, such as airglow and auroras. It was first proposed in 1956 by Donald M. Hunten, Franklin E. Roach, and Joseph W. Chamberlain.^[1] It is named for Robert Strutt, 4th Baron Rayleigh (1875–1947).^[2] Its symbol is R (also used for the röntgen, an unrelated unit). 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. A column is one centimeter cross-section.^[3] The rayleigh is a unit of an apparent emission rate, without allowances being made for scattering or absorption. The night sky has an intensity of about 250 R, while auroras can reach values of 1000 kR.

The relationship between photon radiance, L, (with unit photon per square metre per second per steradian) and I (with unit rayleigh) is:^{[dubious – discuss]} $I=4\pi ~\mathrm {sr} \times L\times {\frac {\mathrm {R} }{\mathrm {10^{10}~photon{\cdot }m^{-2}{\cdot }s^{-1}} }}$

1 rayleigh can thus be expressed in SI units as either:^[3]

10¹⁰ photons s^-1 (m² column)^-1
1/4π 10¹⁰ photons s^-1 m^-2 sr^-1

References

^ Hunten, D. M.; Roach, F. E.; Chamberlain, J. W. (1956). "A photometric unit for the airglow and aurora". Journal of Atmospheric and Terrestrial Physics. 8 (6): 345–346. Bibcode:1956JATP....8..345H. doi:10.1016/0021-9169(56)90111-8.
^ Baker, Doran J. (1974). "Rayleigh, the Unit for Light Radiance". Applied Optics. 13 (9): 2160–2163. Bibcode:1974ApOpt..13.2160B. doi:10.1364/AO.13.002160. PMID 20134644.
^ ^a ^b Doran J. Baker; Gerald J. Romick. "The rayleigh: interpretation of the unit in terms of column emission rate or apparent radiance expressed in SI units" (PDF).

[1] Hunten, D. M.; Roach, F. E.; Chamberlain, J. W. (1956). "A photometric unit for the airglow and aurora". Journal of Atmospheric and Terrestrial Physics. 8 (6): 345–346. Bibcode:1956JATP....8..345H. doi:10.1016/0021-9169(56)90111-8.

[2] Baker, Doran J. (1974). "Rayleigh, the Unit for Light Radiance". Applied Optics. 13 (9): 2160–2163. Bibcode:1974ApOpt..13.2160B. doi:10.1364/AO.13.002160. PMID 20134644.

[Baker-3] Doran J. Baker; Gerald J. Romick. "The rayleigh: interpretation of the unit in terms of column emission rate or apparent radiance expressed in SI units" (PDF).

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 The '''rayleigh''' is a unit of [[photon]] [[flux]], used to measure faint light emitted in the sky, such as [[airglow]] and [[Aurora (astronomy)|aurora]]s. It was first proposed in 1956 by [[Donald M. Hunten]], [[Franklin E. Roach]], and [[Joseph W. Chamberlain]].<ref>{{cite journal | author1 = Hunten, D. M. | author2-link = Franklin E. Roach | author2 = Roach, F. E. | author3 = Chamberlain, J. W. | year = 1956 | title = A photometric unit for the airglow and aurora | journal = Journal of Atmospheric and Terrestrial Physics | volume = 8 | pages = 345–346 | doi = 10.1016/0021-9169(56)90111-8 | issue = 6 | bibcode = 1956JATP....8..345H }}</ref> It is named for [[Robert Strutt, 4th Baron Rayleigh]] (1875–1947).<ref>{{cite journal | doi = 10.1364/AO.13.002160 | first = Doran J. | last = Baker | title = Rayleigh, the Unit for Light Radiance | journal = Applied Optics | volume = 13 | issue = 9 | pages = 2160–2163 | year = 1974 | url = http://www.opticsinfobase.org/abstract.cfm?URI=ao-13-9-2160 | pmid = 20134644 | bibcode = 1974ApOpt..13.2160B }}</ref> Its symbol is R (also used for the [[Roentgen (unit)|röntgen]], an unrelated unit). [[SI prefix]]es are used with the rayleigh.