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Walsh–Hadamard Angle Transform

Updated 1 February 2026
  • Walsh–Hadamard Angle Transform is a discrete integral transform that decomposes angular signals into binary square-wave components using Walsh–Hadamard basis functions.
  • It leverages a hybrid classical–quantum framework to achieve O(N) computational complexity, significantly improving processing speed over classical methods.
  • The transform employs precise polar discretization with uniform-area and uniform-radial subdivisions to maintain orthogonality and enable effective image artifact removal.

The Walsh–Hadamard Angle Transform (WAT) is a discrete integral transform operating on angular coordinate samples using Walsh–Hadamard basis functions. Developed as part of a hybrid classical–quantum framework for image processing in polar coordinates, WAT decomposes angular functions into binary-valued “square-wave” components of varying sequency. The transform’s capabilities include the denoising of artifacts such as circular and azimuthal banding in images and applications to optical system diagnostics, medical imaging, and radar/sonar polar mappings. Efficient quantum algorithms, building on earlier Walsh–Hadamard transform work, offer a computational complexity of O(N)\mathcal{O}(N), improving upon the classical fast Walsh–Hadamard transform (O(Nlog2N)\mathcal{O}(N \log_2 N)) (Rohida et al., 2024).

1. Polar Walsh Basis Functions and Discretization

Walsh basis functions in polar coordinates are constructed on a disk of radius rmaxr_{\max}, partitioned into Nr=2nrN_r = 2^{n_r} radial divisions and Nθ=2nθN_\theta = 2^{n_\theta} angular sectors. Two subdivision schemes are defined:

  • Uniform-area subdivision (f=12f = \tfrac{1}{2}): rk=rmax[(k+1)/Nr]1/2r_k = r_{\max} \left[(k+1)/N_r \right]^{1/2}
  • Uniform-radial subdivision (f=1f = 1): rk=rmax[(k+1)/Nr]r_k = r_{\max} \left[(k+1)/N_r \right]

Angular nodes are similarly given by θ=2π(+1/2)/Nθ\theta_\ell = 2\pi (\ell+1/2)/N_\theta for O(Nlog2N)\mathcal{O}(N \log_2 N)0. Each annular–sector cell O(Nlog2N)\mathcal{O}(N \log_2 N)1 contains a constant-valued polar Walsh function. Two function orders are defined:

  • Natural-order: O(Nlog2N)\mathcal{O}(N \log_2 N)2
  • Sequency-order: O(Nlog2N)\mathcal{O}(N \log_2 N)3

The functions factorize into separate radial and angular components: O(Nlog2N)\mathcal{O}(N \log_2 N)4, with O(Nlog2N)\mathcal{O}(N \log_2 N)5 and O(Nlog2N)\mathcal{O}(N \log_2 N)6 in natural order (Rohida et al., 2024).

2. Orthogonality and Normalization

Orthogonality of the Walsh basis holds both discretely and approximately in the continuous limit:

  • Discrete orthogonality:

O(Nlog2N)\mathcal{O}(N \log_2 N)7

The orthonormal set is O(Nlog2N)\mathcal{O}(N \log_2 N)8.

  • Continuous approximation:

O(Nlog2N)\mathcal{O}(N \log_2 N)9

Appropriate rmaxr_{\max}0-weighting may be introduced depending on subdivision choice (rmaxr_{\max}1).

This rigorous structure underpins transform invertibility and spectrum sparsity properties (Rohida et al., 2024).

3. Walsh–Hadamard Angle Transform Kernel

The 1D Walsh–Hadamard transform matrix rmaxr_{\max}2 of size rmaxr_{\max}3 is defined via entries

rmaxr_{\max}4

where rmaxr_{\max}5.

Given an angular signal rmaxr_{\max}6, for instance a pixel value at fixed radius versus angle, its WAT is

rmaxr_{\max}7

for rmaxr_{\max}8, or in vector notation rmaxr_{\max}9. The inverse is Nr=2nrN_r = 2^{n_r}0 since Nr=2nrN_r = 2^{n_r}1. In sequency order, the bit transform of Nr=2nrN_r = 2^{n_r}2 is utilized (Rohida et al., 2024).

The transform decomposes Nr=2nrN_r = 2^{n_r}3 into angular “square-wave” functions of increasing sequency, with low Nr=2nrN_r = 2^{n_r}4 indexing smooth angular features and high Nr=2nrN_r = 2^{n_r}5 encoding rapid oscillations.

4. Hybrid Classical–Quantum Implementation and Complexity

A two-dimensional WAT (across both radius and angle) is realized as Nr=2nrN_r = 2^{n_r}6 for an image Nr=2nrN_r = 2^{n_r}7 of size Nr=2nrN_r = 2^{n_r}8. A hybrid classical–quantum algorithm leverages quantum Hadamard operations to achieve cost Nr=2nrN_r = 2^{n_r}9 for Nθ=2nθN_\theta = 2^{n_\theta}0, outperforming the classical fast Walsh–Hadamard transform’s Nθ=2nθN_\theta = 2^{n_\theta}1.

PolarQWHT(X) Procedure

  1. Apply 1D Walsh–Hadamard transform to each angular column at fixed radius.
  2. Apply 1D Walsh–Hadamard transform to each row (angularized) on the result.
  3. Each 1D transform QWHT_1d is implemented by:
    • State preparation (classical, Nθ=2nθN_\theta = 2^{n_\theta}2)
    • Hadamard gate layer (quantum, depth 1, Nθ=2nθN_\theta = 2^{n_\theta}3)
    • Measurement, sign correction, and Walsh spectrum reconstruction The sign correction uses the classical “delta-shift trick” (Rohida et al., 2024).

Quantum circuit steps include Nθ=2nθN_\theta = 2^{n_\theta}4 classical preprocessing/postprocessing, parallel Hadamard gates, Nθ=2nθN_\theta = 2^{n_\theta}5 shots for output probability estimation, and classical sign correction.

5. Practical Applications: Image Denoising and Diagnostic Imaging

The WAT framework enables efficient removal of structured noise in polar images. For example, azimuthal banding artifacts can be suppressed by:

  • Transforming a noisy angular profile Nθ=2nθN_\theta = 2^{n_\theta}6 noise using Nθ=2nθN_\theta = 2^{n_\theta}7
  • Suppressing components at specific sequency Nθ=2nθN_\theta = 2^{n_\theta}8, then reconstructing the cleansed angular profile by inverse transform

Full-image artifact removal involves Cartesian-to-polar mapping, PolarQWHT application, selective H-domain filtering, inverse transform, and interpolation back to Cartesian coordinates. The spectrum before and after demonstrates targeted suppression of banding noise (Rohida et al., 2024).

Applications span:

  • Optical system diagnostics (e.g., Airy pattern removal)
  • Astronomical imaging
  • Medical CT ring artifact reduction
  • Sonar and radar polar mapping

6. Practical Considerations and Limitations

Key consideration include:

  • Interpolation challenges: Cartesian-to-polar conversion requires averaging or bilinear interpolation, balancing smoothing with aliasing risk.
  • Sampling uniformity: Uniform-area subdivision (Nθ=2nθN_\theta = 2^{n_\theta}9) equalizes pixel density across annuli, stabilizing sampling.
  • Quantum measurement noise: Obtaining accurate WHT coefficients necessitates many shots and error mitigation.
  • Restrictive grid sizes: Both f=12f = \tfrac{1}{2}0 and f=12f = \tfrac{1}{2}1 must be powers of two.
  • Polar grid artifacts: Non-injective mapping leads to edge artifacts, especially near the disk center and perimeter.
  • Current hybrid limitations: There is an f=12f = \tfrac{1}{2}2 classical overhead for quantum state preparation and sign correction (Rohida et al., 2024).

7. Extensions and Open Research Questions

Proposed extensions and outstanding problems include:

  • Development of continuous, analytic polar Walsh–Hadamard transforms amendable to fast hardware
  • Explicit error bounds for interpolation and QWHT sign recovery in the presence of realistic noise
  • Generalization to non-uniform angular and radial grids
  • Exploration of richer radial bases and non-binary subdivisions
  • Hybrid transforms blending Fourier and Walsh–Hadamard methods

A plausible implication is that such developments could expand applicability and further reduce computational overheads for large-scale polar image processing tasks (Rohida et al., 2024).

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