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Beer–Lambert law

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In optics, the Beer-Lambert law, also known as Beer's law or the Lambert-Beer law or the Beer-Lambert-Bouguer law is an empirical relationship that relates the absorption of light to the properties of the material through which the light is travelling.

Equations

File:Beer lambert.png
Diagram of Beer-Lambert absorption of a beam of light as it travels through a cuvette of size l.

There are several ways in which the law can be expressed:

Here:

In essence, the law states that there is a logarithmic dependence between the transmission of light through a substance and the concentration of the substance, and also between the transmission and the length of material that the light travels through. Thus if l and α are known, the concentration of a substance can be deduced from the amount of light transmitted by it.

The units of c and α depend on the way that the concentration of the absorber is being expressed. If the material is a liquid, it is usual to express the absorber concentration c as a mole fraction i.e. a dimensionless fraction. The units of α are thus reciprocal length (e.g. cm-1). In the case of a gas, c may be expressed as a density (units of reciprocal length cubed, e.g. cm-3), in which case α is an absorption cross-section and has units of length squared (e.g. cm²). If concentration c is expressed in moles per unit volume, α is a molar absorptivity (usually given the symbol ε) in units of mol-1 cm-2 or sometimes L mol-1 cm-1.

The value of the absorption coefficient α varies between different absorbing materials and also with wavelength for a particular material. It is usually determined by experiment.

In spectroscopy and spectrophotometry, the law is almost always defined in terms of common logarithms and powers of 10 as above. In general optics, the law is often defined in an alternate exponential form:

The values of α' and A' are approximately 2.3 (≈ln 10) times larger than the corresponding values of α and A defined in terms of base-10 functions. Therefore, care must be taken when interpreting data that the correct form of the law is used.

The law tends to break down at very high concentrations, especially if the material is highly scattering. If the light is especially intense, nonlinear optical processes can also cause variances.

Derivation

Assume that particles may be described as having an area, , perpendicular to the path of light through a solution, such that a photon of light is absorbed if it strikes the particle, and is transmitted if it does not.

Define as an axis parallel to the direction that photons of light are moving, '' and '' are the area and thickness (along the axis) of a 3-dimensional slab of space through which light is passing. We assume that is sufficiently small that one particle in the slab cannot obscure another particle in the slab when viewed along the direction. The concentration of particles in the slab is represented by ‘’.

It follows that the fraction of photons absorbed when passing through this slab is equal to the total opaque area of the particles in the slab, , divided by the area of the slab, or . Expressing the number of photons absorbed by the slab as , and the total number of photons incident on the slab as , the fraction of photons absorbed by the slab is given by

The solution to this simple differential equation is obtained by integrating both sides to obtain as a function of

For a slab of real thickness, ‘’, the difference in light intensity at z=0, and at z=l, is given by

or

Beer-Lambert law in the atmosphere

This law is also applied to describe the attenuation of solar radiation as it travels through the atmosphere. In this case, there is scattering of radiation as well as absorption. The Beer-Lambert law for the atmosphere is usually written

,

where each is an extinction coefficient whose subscript identifies the source of the absorption or scattering it describes:

  • refers to aerosols (that absorb and scatter)
  • are uniformly mixed gases (mainly carbon dioxide () and molecular oxygen () which only absorb)
  • is nitrogen dioxide, mainly due to urban pollution (absorption only)
  • is water vapour absorption
  • is ozone (absorption only)
  • is Rayleigh scattering from molecular oxygen () and nitrogen () (responsible for the blue color of the sky).

is the optical mass, a term basically equal to where is the solar zenith angle (the solar angle with respect to a direction perpendicular to the Earth's surface at the observation site).

This equation can be used to retrieve , the aerosol optical thickness, which is necessary for the correction of satellite images and also important in accounting for the role of aerosols in climate.

History

The law was independently discovered (in various forms) by Pierre Bouguer in 1729, Johann Heinrich Lambert in 1760 and August Beer in 1852.

See also