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Coherence length

Distance over which a propagating wave maintains a certain degree of coherence

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Through Physics, Coherence (physics) and Electromagnetic radiation

This article focuses on the coherence of classical electromagnetic fields. In quantum mechanics, there is a mathematically analogous concept of the quantum coherence length of a wave function.

Formulas

In radio-band systems, the coherence length is approximated by

L=cnΔf≈λ2nΔλ,

where c is the speed of light in vacuum, n is the refractive index of the medium, and Δf is the bandwidth of the source or λ is the signal wavelength and Δλ is the width of the range of wavelengths in the signal.

In optical communications and optical coherence tomography (OCT), assuming that the source has a Gaussian emission spectrum, the roundtrip coherence length L is given by

L=2ln⁡2πλ2ngΔλ,

where λ is the central wavelength of the source, ng is the group refractive index of the medium, and Δλ is the (FWHM) spectral width of the source. If the source has a Gaussian spectrum with FWHM spectral width Δλ, then a path offset of ±L will reduce the fringe visibility to 50%. This is a roundtrip coherence length; this definition is applied in applications like OCT where the light traverses the measured displacement twice (as in a Michelson interferometer). In transmissive applications, such as with a Mach–Zehnder interferometer, the light traverses the displacement only once, and the coherence length is effectively doubled.

The coherence length can also be measured using a Michelson interferometer and is the optical path length difference of a self-interfering laser beam which corresponds to 1e≈37% fringe visibility, where the fringe visibility is defined as

V=Imax−IminImax+Imin,

where I is the fringe intensity.

In long-distance transmission systems, the coherence length may be reduced by propagation factors such as dispersion, scattering, and diffraction.

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