In radiometry, radiant exposure or fluence is the radiant energy received by a surface per unit area, or equivalently the irradiance of a surface, integrated over time of irradiation, and spectral exposure is the radiant exposure per unit frequency or wavelength, depending on whether the spectrum is taken as a function of frequency or of wavelength. The SI unit of radiant exposure is the joule per square metre (J/m2), while that of spectral exposure in frequency is the joule per square metre per hertz (J⋅m−2⋅Hz−1) and that of spectral exposure in wavelength is the joule per square metre per metre (J/m3)—commonly the joule per square metre per nanometre (J⋅m−2⋅nm−1).

Mathematical definitions

Radiant exposure

Radiant exposure of a surface, denoted He ("e" for "energetic", to avoid confusion with photometric quantities), is defined as H e = ∂ Q e ∂ A = ∫ 0 T E e ( t ) d t , {\displaystyle H_{\mathrm {e} }={\frac {\partial Q_{\mathrm {e} }}{\partial A}}=\int _{0}^{T}E_{\mathrm {e} }(t)\,\mathrm {d} t,} where

  • ∂ is the partial derivative symbol;
  • Qe is the radiant energy;
  • A is the area;
  • T is the duration of irradiation;
  • Ee is the irradiance.

Spectral exposure

Spectral exposure in frequency of a surface, denoted He,ν, is defined as H e , ν = ∂ H e ∂ ν , {\displaystyle H_{\mathrm {e} ,\nu }={\frac {\partial H_{\mathrm {e} }}{\partial \nu }},} where ν is the frequency.

Spectral exposure in wavelength of a surface, denoted He,λ, is defined as H e , λ = ∂ H e ∂ λ , {\displaystyle H_{\mathrm {e} ,\lambda }={\frac {\partial H_{\mathrm {e} }}{\partial \lambda }},} where λ is the wavelength.

SI radiometry units

SI radiometry unitsvte
QuantityUnitDimensionNotes
NameSymbolNameSymbol
Radiant energyQejouleJML2⋅T−2Energy of electromagnetic radiation.
Radiant energy densitywejoule per cubic metreJ/m3ML−1⋅T−2Radiant energy per unit volume.
Radiant fluxΦewattW = J/sML2⋅T−3Radiant energy emitted, reflected, transmitted or received, per unit time. This is sometimes also called "radiant power", and called luminosity in astronomy.
Spectral fluxΦe,νwatt per hertzW/HzML2⋅T−2Radiant flux per unit frequency or wavelength. The latter is commonly measured in W⋅nm−1.
Φe,λwatt per metreW/mMLT−3
Radiant intensityIe,Ωwatt per steradianW/srML2⋅T−3Radiant flux emitted, reflected, transmitted or received, per unit solid angle. This is a directional quantity.
Spectral intensityIe,Ω,νwatt per steradian per hertzW⋅sr−1⋅Hz−1ML2⋅T−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,λwatt per steradian per metreW⋅sr−1⋅m−1MLT−3
RadianceLe,Ωwatt 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 called "intensity".
Spectral radiance Specific intensityLe,Ω,νwatt 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 called "spectral intensity".
Le,Ω,λwatt per steradian per square metre, per metreW⋅sr−1⋅m−3ML−1⋅T−3
Irradiance Flux densityEewatt per square metreW/m2MT−3Radiant flux received by a surface per unit area. This is sometimes also called "intensity".
Spectral irradiance Spectral flux densityEe,νwatt per square metre per hertzW⋅m−2⋅Hz−1MT−2Irradiance of a surface per unit frequency or wavelength. This is sometimes also 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,λwatt per square metre, per metreW/m3ML−1⋅T−3
RadiosityJewatt per square metreW/m2MT−3Radiant flux leaving (emitted, reflected and transmitted by) a surface per unit area. This is sometimes also called "intensity".
Spectral radiosityJe,νwatt 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 called "spectral intensity".
Je,λwatt per square metre, per metreW/m3ML−1⋅T−3
Radiant exitanceMewatt 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 called "intensity".
Spectral exitanceMe,νwatt 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 called "spectral intensity".
Me,λwatt per square metre, per metreW/m3ML−1⋅T−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,νjoule 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,λjoule per square metre, per metreJ/m3ML−1⋅T−2
See also: SIRadiometryPhotometry

See also