Coherence Area
Understanding Coherence Area
When a radio wave propagates through free space from a point source, the wavefront at any distance is a perfect sphere (or approximately a plane wave at large distances), and the field is perfectly coherent across any transverse plane: every point on the wavefront has a fixed, predictable phase relationship to every other point. But when the source is extended (subtending a finite angle), or when scattering creates multiple effective sources, different parts of the transverse plane receive contributions from different source directions, and the phase relationships become random beyond a certain spatial scale. This scale defines the coherence area.
The concept connects optics and RF engineering. In optics, coherence area determines the resolution of interferometers and the fringe visibility of double-slit experiments. In RF, it determines how large an antenna aperture can be used effectively, how far apart MIMO antennas must be spaced for independent channels, and how many spatial degrees of freedom a propagation environment provides. Understanding coherence area is fundamental to designing antenna arrays, massive MIMO systems, and radio interferometers.
Coherence Area Formulas
rc = 0.61 λ / θs
Coherence Area:
Ac = π rc² = π (0.61 λ / θs)²
MIMO Spatial Degrees of Freedom:
Ndof ≈ Aarray / Ac
Where θs = source angular extent (rad), λ = wavelength. At 2 GHz (λ = 0.15 m), θs = 10° (0.175 rad): rc = 0.52 m. Urban isotropic (θs = 2π): rc ≈ λ/(2π) ≈ 0.024 m, Ac ≈ 0.0018 m².
Coherence Area in RF Environments
| Environment | θs | rc at 2 GHz | Ac | MIMO Impact |
|---|---|---|---|---|
| Satellite (GEO) | <0.01° | >500 m | >800,000 m² | No spatial diversity |
| Rural LOS | 2 to 5° | 1 to 3 m | 3 to 28 m² | Limited MIMO |
| Suburban | 30 to 60° | 0.1 to 0.3 m | 0.03 to 0.3 m² | Good MIMO |
| Urban NLOS | 120 to 360° | 0.024 to 0.07 m | 0.002 to 0.015 m² | Excellent MIMO |
| Indoor rich scatter | ≈360° | ≈λ/2π | ≈λ²/4π | Maximum diversity |
Frequently Asked Questions
How does coherence area relate to antenna gain?
Antenna gain requires coherent wavefront across aperture. If Ac < Aphys, effective aperture limited to Ac, reducing gain. Satellite links: coherent across huge apertures (point source). Urban: Ac ≈ few λ², so massive MIMO works (array much larger than coherence area, each element sees independent fading).
What is the van Cittert-Zernike theorem?
Spatial coherence = normalized Fourier transform of source intensity distribution. Circular source: μ(d) = 2J1(πdθs/λ)/(πdθs/λ). First zero at d = 1.22λ/θs. Point source: infinite coherence. 10° source at 1 GHz: rc = 2.1 m, Ac ≈ 14 m².
How does it affect MIMO?
MIMO needs independent fading at each antenna: spacing ≥ coherence distance. Rich scattering (θs ≈ 360°): rc ≈ λ/2, so standard λ/2 spacing works. Limited scattering (rural LOS): rc = meters, need much wider spacing. Determines channel matrix rank: Ac > array = rank 1 (no MIMO gain).