Coherence length

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In physics, coherence length is the propagation distance over which a coherent wave (e.g. an electromagnetic wave) maintains a specified degree of coherence. Wave interference is strong when the paths taken by all of the interfering waves differ by less than the coherence length. A wave with a longer coherence length is closer to a perfect sinusoidal wave. Coherence length is important in holography and telecommunications engineering. 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=cnΔfλ2nΔλ,

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=2ln2πλ2ngΔλ,[1][2]

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%. It is important to note that 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 1e37% fringe visibility,[3] where the fringe visibility is defined as

V=ImaxIminImax+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.

Lasers

Multimode helium–neon lasers have a typical coherence length on the order of centimeters, while the coherence length of longitudinally single-mode lasers can exceed 1 km. Semiconductor lasers can reach some 100 m, but small, inexpensive semiconductor lasers have shorter lengths, with one source[4] claiming 20 cm. Singlemode fiber lasers with linewidths of a few kHz can have coherence lengths exceeding 100 km. Similar coherence lengths can be reached with optical frequency combs due to the narrow linewidth of each tooth. Non-zero visibility is present only for short intervals of pulses repeated after cavity length distances up to this long coherence length.

Other light sources

Tolansky's An introduction to Interferometry has a chapter on sources which quotes a line width of around 0.052 angstroms for each of the Sodium D lines in an uncooled low-pressure sodium lamp, corresponding to a coherence length of around 67 mm for each line by itself.[5] Cooling the low pressure sodium discharge to liquid nitrogen temperatures increases the individual D line coherence length by a factor of 6. A very narrow-band interference filter would be required to isolate an individual D line.

See also

References

  1. Akcay, C.; Parrein, P.; Rolland, J.P. (2002). "Estimation of longitudinal resolution in optical coherence imaging". Applied Optics. 41 (25): 5256–5262. Bibcode:2002ApOpt..41.5256A. doi:10.1364/ao.41.005256. PMID 12211551. equation 8
  2. Izatt; Choma; Dhalla (2014). "Theory of Optical Coherence Tomography". In Drexler; Fujimoto (eds.). Optical Coherence Tomography. Springer Berlin Heidelberg. ISBN 978-3-319-06419-2.
  3. Ackermann, Gerhard K. (2007). Holography: A Practical Approach. Wiley-VCH. ISBN 978-3-527-40663-0.
  4. "Sam's Laser FAQ - Diode Lasers". www.repairfaq.org. Retrieved 2017-02-06.
  5. Tolansky, Samuel (1973). An Introduction to Interferometry. Longman. ISBN 9780582443334.