Electromagnetic Theory

Coherency Matrix

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The coherency matrix J is a 2×2 Hermitian matrix describing the full second-order polarization state of an EM wave, including partially polarized signals. Jij = ⟨EiEj*⟩. Degree of polarization p = √(1 - 4 det(J)/tr(J)²). Related to Stokes: S0 = J11+J22, S1 = J11-J22, S2 = 2Re(J12), S3 = 2Im(J12). Used in polarimetric radar for Cloude-Pottier target decomposition.
Category: Electromagnetic Theory
Size: 2×2 Hermitian
Parameters: 4 real (= Stokes)

Understanding the Coherency Matrix

Polarization is a fundamental property of electromagnetic waves, and its complete description requires more than just stating "horizontal" or "circular." Real-world RF signals are often partially polarized: a combination of a deterministic (polarized) component and a random (unpolarized) component. This arises from multipath propagation, rough surface scattering, thermal emission, and mixing of independent sources. The coherency matrix captures this complexity in a compact 2×2 matrix that separates the polarized and unpolarized contributions through its eigenvalue decomposition.

The matrix framework connects to multiple representation systems used in different RF engineering disciplines. Antenna engineers use Jones vectors and matrices for fully polarized signals through deterministic systems. Radiometer engineers use Stokes parameters for power-based measurements of partially polarized thermal emission. Polarimetric radar engineers use scattering matrices and target decomposition theorems. The coherency matrix unifies these: Jones vectors are its rank-1 case, Stokes parameters are linear combinations of its elements, and target decomposition operates on its 3×3 generalization.

Coherency Matrix Equations

Coherency Matrix:
J = ⟨E EH⟩ = [[⟨|Ex|²⟩, ⟨ExEy*⟩], [⟨EyEx*⟩, ⟨|Ey|²⟩]]

Degree of Polarization:
p = √(1 - 4 det(J) / tr(J)²) = (λ1 - λ2) / (λ1 + λ2)

Stokes from Coherency:
S = [J11+J22, J11-J22, 2Re(J12), 2Im(J12)]

Where λ1 ≥ λ2 ≥ 0 are eigenvalues. Fully polarized: det(J) = 0, p = 1. Unpolarized: J = (P/2)I, p = 0. Partially polarized: 0 < p < 1. Total power = tr(J) = S0.

Polarization State Examples

StateCoherency MatrixpStokesSource
Horizontal linear[[1,0],[0,0]]1[1,1,0,0]Dipole antenna
RHCP½[[1,-j],[j,1]]1[1,0,0,1]Helix antenna
Unpolarized½[[1,0],[0,1]]0[1,0,0,0]Thermal emission
50% polarized H[[0.75,0],[0,0.25]]0.5[1,0.5,0,0]Ground reflection
45° linear½[[1,1],[1,1]]1[1,0,1,0]Rotated dipole
Common Questions

Frequently Asked Questions

How does it describe partial polarization?

Fully polarized: rank 1 (det = 0, one zero eigenvalue), p = 1. Unpolarized: J ∝ I (equal eigenvalues), p = 0. Partially polarized: eigenvalue decomposition uniquely separates polarized + unpolarized components. p = (λ12)/(λ12). Multipath, rough scattering, thermal emission produce 0 < p < 1.

How is it used in polarimetric radar?

Scattering matrix S → Pauli vector k → 3×3 coherency matrix T = ⟨kkH⟩. Cloude-Pottier decomposition: eigenvalues/eigenvectors classify scatterers (surface, volume, double-bounce). Applications: SAR land cover mapping, crop monitoring, forest biomass, disaster assessment.

Relationship to Stokes parameters?

Linear transformation: S0=J11+J22, S1=J11-J22, S2=2Re(J12), S3=2Im(J12). Equivalent information. Stokes: measurable with power detectors (radiometry). Coherency: preserves complex field (radar, interferometry). p = √(S1²+S2²+S3²)/S0 = √(1-4det(J)/tr(J)²).

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