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Coherence Length

Coherence length is the maximum distance over which light waves stay "in step" with each other. If two waves travel different paths longer than this, they lose their fixed phase relationship and can no longer produce clear interference. Lasers have very long coherence lengths (metres or more), while ordinary light bulbs have very short ones (micrometres). This is why lasers are used for holography and interferometry. It is calculated from the wavelength and the spectral width of the light.

Optics Wave Optics Coherence

Coherence Length CalculatorLc = λ² / Δλ

Lc = λ² / Δλ
Lc = coherence length (m)  ·  λ = wavelength (m)  ·  Δλ = spectral width (m)
⟹ Solve⟷Lc, λ, Δλ
m
m
m
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Coherence Length—
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Lc: —λ: —Δλ: —
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Coherence Length (log scale)—
Short (< 0.1 m) Medium (0.1–10 m) Long (> 10 m)
Lc = λ² / Δλ  ·  Coherence length is the distance over which a wave maintains a constant phase relation.

Variables

Symbol Quantity Unit
Lc Coherence length m
λ Central wavelength m
Δλ Spectral bandwidth m

What it means

Coherence length is a measure of the temporal coherence of a light source. It is inversely proportional to the spectral width (Δλ). A longer coherence length allows more interference fringes and is needed for high‑precision interferometry. Lasers have long coherence lengths; LEDs have short. Understanding this is essential for designing interferometers, holography systems, and in fibre optic communications where phase coherence matters.

Worked example

Coherence Length – Two Detailed Examples

Real‑World
Scenario: A HeNe laser has wavelength λ = 632.8 nm and spectral linewidth Δλ = 0.002 nm. The coherence length Lc = λ² / Δλ = (632.8²) / 0.002 = 400,000 nm? Actually 632.8 nm squared = 400,000 nm²? Let's compute: λ² = (632.8e-9)² = 4.00e-13 m², Δλ = 0.002e-9 m, so Lc = 4.00e-13 / 0.002e-9 = 2.00e-4 m = 0.2 m = 200 mm. The laser light remains coherent over a distance of about 20 cm, which is sufficient for many interferometric applications. The physicist uses this to design a Michelson interferometer with path differences less than the coherence length to observe interference fringes.
ParameterValue
λ (nm)632.8
Δλ (nm)0.002
1Lc = (632.8e-9)² / (0.002e-9) = 4.00e-13 / 2e-12 = 0.2 m
Result 0.2 m ✓ Coherence length
Scenario: An LED emits at 850 nm with a spectral width of 10 nm. The coherence length Lc = (850²) / 10 = 72250 nm? Compute: λ² = (850e-9)² = 7.225e-13 m², Δλ = 10e-9 m, Lc = 7.225e-13 / 1e-8 = 7.225e-5 m ≈ 72 µm. This short coherence length means that the LED light is incoherent over even a short path difference, making it unsuitable for interferometry but excellent for illumination and communications.
ParameterValue
λ850
Δλ10
1Lc = (850e-9)² / (10e-9) = 7.225e-13 / 1e-8 = 7.225e-5 m ≈ 72 µm
Result 72 µm ✓ Short coherence
Insight: Coherence length is inversely proportional to spectral linewidth. A narrow linewidth gives long coherence length, essential for high‑precision interferometry. Conversely, broad linewidth sources have short coherence and are used in coherence‑domain imaging.

Common mistakes

  • Coherence length: L_c = λ² / Δλ – where Δλ is the spectral width of the source.
  • Units: λ and Δλ in the same units (e.g., nm) – L_c in the same unit.
  • Interpretation: The distance over which the light remains coherent – for a laser, L_c can be long; for an LED, short.
  • Assumes: Gaussian or rectangular spectrum – this is an approximation.
  • Coherence time: τ_c = L_c / c – the corresponding time.

Applications

Coherence length, L_c = λ²/Δλ, is the distance over which a light wave maintains a predictable phase relationship, limited by the spectral width Δλ. This is important in interferometry, holography, and optical communications. Engineers use it to select light sources for coherence‑dependent applications. For example, laser sources have long coherence lengths, suitable for interferometry, while LEDs have short coherence lengths, reducing speckle. By understanding coherence length, they can design systems for optical coherence tomography (OCT), fibre sensors, and metrology. This concept is fundamental to understanding the temporal coherence of light.

  • Design of interferometers and holographic systems
  • Optical coherence tomography (OCT) for medical imaging
  • Selection of light sources for coherence‑sensitive applications
  • Speckle reduction in imaging and display systems
  • Understanding of laser and light source characteristics