Wall-plug efficiency

In optics, wall-plug efficiency or radiant efficiency is the energy conversion efficiency with which the system converts electrical power into optical power. It is defined as the ratio of the radiant flux (i.e., the total optical output power) to the input electrical power.[1]

In laser systems, this efficiency includes losses in the power supply and also the power required for a cooling system, not just the laser itself.[2]

See also

References

QuantityUnitDimensionNotes
NameSymbol[nb 1]NameSymbol
Radiant energyQe[nb 2]jouleJML2T−2Energy of electromagnetic radiation.
Radiant energy densitywejoule per cubic metreJ/m3ML−1T−2Radiant energy per unit volume.
Radiant fluxΦe[nb 2]wattW = J/sML2T−3Radiant energy emitted, reflected, transmitted or received, per unit time. This is sometimes also called "radiant power", and called luminosity in Astronomy.
Spectral fluxΦe,ν[nb 3]watt per hertzW/HzML2T −2Radiant flux per unit frequency or wavelength. The latter is commonly measured in W⋅nm−1.
Φe,λ[nb 4]watt per metreW/mMLT−3
Radiant intensityIe,Ω[nb 5]watt per steradianW/srML2T−3Radiant flux emitted, reflected, transmitted or received, per unit solid angle. This is a directional quantity.
Spectral intensityIe,Ω,ν[nb 3]watt per steradian per hertzW⋅sr−1⋅Hz−1ML2T−2Radiant intensity per unit frequency or wavelength. The latter is commonly measured in W⋅sr−1⋅nm−1. This is a directional quantity.
Ie,Ω,λ[nb 4]watt per steradian per metreW⋅sr−1⋅m−1MLT−3
RadianceLe,Ω[nb 5]watt per steradian per square metreW⋅sr−1⋅m−2MT−3Radiant flux emitted, reflected, transmitted or received by a surface, per unit solid angle per unit projected area. This is a directional quantity. This is sometimes also confusingly called "intensity".
Spectral radiance
Specific intensity
Le,Ω,ν[nb 3]watt per steradian per square metre per hertzW⋅sr−1⋅m−2⋅Hz−1MT−2Radiance of a surface per unit frequency or wavelength. The latter is commonly measured in W⋅sr−1⋅m−2⋅nm−1. This is a directional quantity. This is sometimes also confusingly called "spectral intensity".
Le,Ω,λ[nb 4]watt per steradian per square metre, per metreW⋅sr−1⋅m−3ML−1T−3
Irradiance
Flux density
Ee[nb 2]watt per square metreW/m2MT−3Radiant flux received by a surface per unit area. This is sometimes also confusingly called "intensity".
Spectral irradiance
Spectral flux density
Ee,ν[nb 3]watt per square metre per hertzW⋅m−2⋅Hz−1MT−2Irradiance of a surface per unit frequency or wavelength. This is sometimes also confusingly called "spectral intensity". Non-SI units of spectral flux density include jansky (1 Jy = 10−26 W⋅m−2⋅Hz−1) and solar flux unit (1 sfu = 10−22 W⋅m−2⋅Hz−1 = 104 Jy).
Ee,λ[nb 4]watt per square metre, per metreW/m3ML−1T−3
RadiosityJe[nb 2]watt per square metreW/m2MT−3Radiant flux leaving (emitted, reflected and transmitted by) a surface per unit area. This is sometimes also confusingly called "intensity".
Spectral radiosityJe,ν[nb 3]watt per square metre per hertzW⋅m−2⋅Hz−1MT−2Radiosity of a surface per unit frequency or wavelength. The latter is commonly measured in W⋅m−2⋅nm−1. This is sometimes also confusingly called "spectral intensity".
Je,λ[nb 4]watt per square metre, per metreW/m3ML−1T−3
Radiant exitanceMe[nb 2]watt per square metreW/m2MT−3Radiant flux emitted by a surface per unit area. This is the emitted component of radiosity. "Radiant emittance" is an old term for this quantity. This is sometimes also confusingly called "intensity".
Spectral exitanceMe,ν[nb 3]watt per square metre per hertzW⋅m−2⋅Hz−1MT−2Radiant exitance of a surface per unit frequency or wavelength. The latter is commonly measured in W⋅m−2⋅nm−1. "Spectral emittance" is an old term for this quantity. This is sometimes also confusingly called "spectral intensity".
Me,λ[nb 4]watt per square metre, per metreW/m3ML−1T−3
Radiant exposureHejoule per square metreJ/m2MT−2Radiant energy received by a surface per unit area, or equivalently irradiance of a surface integrated over time of irradiation. This is sometimes also called "radiant fluence".
Spectral exposureHe,ν[nb 3]joule per square metre per hertzJ⋅m−2⋅Hz−1MT−1Radiant exposure of a surface per unit frequency or wavelength. The latter is commonly measured in J⋅m−2⋅nm−1. This is sometimes also called "spectral fluence".
He,λ[nb 4]joule per square metre, per metreJ/m3ML−1T−2
See also:


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