
Thereflectance of the surface of amaterial is its effectiveness inreflectingradiant energy. It is the fraction of incident electromagnetic power that is reflected at the boundary. Reflectance is a component of the response of theelectronic structure of the material to the electromagnetic field of light, and is in general a function of the frequency, orwavelength, of the light, its polarization, and theangle of incidence. The dependence of reflectance on the wavelength is called areflectance spectrum orspectral reflectance curve.
Thehemispherical reflectance of a surface, denotedR, is defined as[1]whereΦer is theradiant fluxreflected by that surface andΦei is the radiant fluxreceived by that surface.
Thespectral hemispherical reflectance in frequency andspectral hemispherical reflectance in wavelength of a surface, denotedRν andRλ respectively, are defined as[1]where
Thedirectional reflectance of a surface, denotedRΩ, is defined as[1]where
This depends on both the reflected direction and the incoming direction. In other words, it has a value for every combination of incoming and outgoing directions. It is related to thebidirectional reflectance distribution function and its upper limit is 1. Another measure of reflectance, depending only on the outgoing direction, isI/F, whereI is the radiance reflected in a given direction andF is the incoming radiance averaged over all directions, in other words, the total flux of radiation hitting the surface per unit area, divided by π.[2] This can be greater than 1 for a glossy surface illuminated by a source such as the sun, with the reflectance measured in the direction of maximum radiance (see alsoSeeliger effect).
Thespectral directional reflectance in frequency andspectral directional reflectance in wavelength of a surface, denotedRΩ,ν andRΩ,λ respectively, are defined as[1]where
Again, one can also define a value ofI/F (see above) for a given wavelength.[3]

For homogeneous and semi-infinite (seehalfspace) materials, reflectivity is the same as reflectance. Reflectivity is the square of the magnitude of theFresnel reflection coefficient,[4]which is the ratio of the reflected to incidentelectric field;[5] as such the reflection coefficient can be expressed as acomplex number as determined by theFresnel equations for a single layer, whereas the reflectance is always a positivereal number.
For layered and finite media, according to theCIE,[citation needed] reflectivity is distinguished fromreflectance by the fact that reflectivity is a value that applies tothick reflecting objects.[6] When reflection occurs from thin layers of material, internal reflection effects can cause the reflectance to vary with surface thickness. Reflectivity is the limit value of reflectance as the sample becomes thick; it is the intrinsic reflectance of the surface, hence irrespective of other parameters such as the reflectance of the rear surface. Another way to interpret this is that the reflectance is the fraction of electromagnetic power reflected from a specific sample, while reflectivity is a property of the material itself, which would be measured on a perfect machine if the material filled half of all space.[7]
Given that reflectance is a directional property, most surfaces can be divided into those that givespecular reflection and those that givediffuse reflection.
For specular surfaces, such as glass or polished metal, reflectance is nearly zero at all angles except at the appropriate reflected angle; that is the same angle with respect to the surface normal in theplane of incidence, but on the opposing side. When the radiation is incident normal to the surface, it is reflected back into the same direction.
For diffuse surfaces, such as matte white paint, reflectance is uniform; radiation is reflected in all angles equally or near-equally. Such surfaces are said to beLambertian.
Most practical objects exhibit a combination of diffuse and specular reflective properties.

Reflection of light occurs at a boundary at which theindex of refraction changes. Specular reflection is calculated by theFresnel equations.[8] Fresnel reflection is directional and therefore does not contribute significantly toalbedo which primarily diffuses reflection.
A liquid surface may be wavy. Reflectance may be adjusted to account forwaviness.
The generalization of reflectance to adiffraction grating, which disperses light bywavelength, is calleddiffraction efficiency.
| Quantity | SI units | Notes | |
|---|---|---|---|
| Name | Sym. | ||
| Hemispherical emissivity | ε | — | Radiant exitance of asurface, divided by that of ablack body at the same temperature as that surface. |
| Spectral hemispherical emissivity | εν ελ | — | Spectral exitance of asurface, divided by that of ablack body at the same temperature as that surface. |
| Directional emissivity | εΩ | — | Radianceemitted by asurface, divided by that emitted by ablack body at the same temperature as that surface. |
| Spectral directional emissivity | εΩ,ν εΩ,λ | — | Spectral radianceemitted by asurface, divided by that of ablack body at the same temperature as that surface. |
| Hemispherical absorptance | A | — | Radiant fluxabsorbed by asurface, divided by that received by that surface. This should not be confused with "absorbance". |
| Spectral hemispherical absorptance | Aν Aλ | — | Spectral fluxabsorbed by asurface, divided by that received by that surface. This should not be confused with "spectral absorbance". |
| Directional absorptance | AΩ | — | Radianceabsorbed by asurface, divided by the radiance incident onto that surface. This should not be confused with "absorbance". |
| Spectral directional absorptance | AΩ,ν AΩ,λ | — | Spectral radianceabsorbed by asurface, divided by the spectral radiance incident onto that surface. This should not be confused with "spectral absorbance". |
| Hemispherical reflectance | R | — | Radiant fluxreflected by asurface, divided by that received by that surface. |
| Spectral hemispherical reflectance | Rν Rλ | — | Spectral fluxreflected by asurface, divided by that received by that surface. |
| Directional reflectance | RΩ | — | Radiancereflected by asurface, divided by that received by that surface. |
| Spectral directional reflectance | RΩ,ν RΩ,λ | — | Spectral radiancereflected by asurface, divided by that received by that surface. |
| Hemispherical transmittance | T | — | Radiant fluxtransmitted by asurface, divided by that received by that surface. |
| Spectral hemispherical transmittance | Tν Tλ | — | Spectral fluxtransmitted by asurface, divided by that received by that surface. |
| Directional transmittance | TΩ | — | Radiancetransmitted by asurface, divided by that received by that surface. |
| Spectral directional transmittance | TΩ,ν TΩ,λ | — | Spectral radiancetransmitted by asurface, divided by that received by that surface. |
| Hemispherical attenuation coefficient | μ | m−1 | Radiant fluxabsorbed andscattered by avolume per unit length, divided by that received by that volume. |
| Spectral hemispherical attenuation coefficient | μν μλ | m−1 | Spectral radiant fluxabsorbed andscattered by avolume per unit length, divided by that received by that volume. |
| Directional attenuation coefficient | μΩ | m−1 | Radianceabsorbed andscattered by avolume per unit length, divided by that received by that volume. |
| Spectral directional attenuation coefficient | μΩ,ν μΩ,λ | m−1 | Spectral radianceabsorbed andscattered by avolume per unit length, divided by that received by that volume. |