Angular Spectrum

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The angular spectrum is a method for representing optical fields as a superposition of plane waves traveling in different directions. It provides an exact solution to the wave equation and is particularly useful for analyzing diffraction and propagation.

Definition

For a monochromatic field $U(x, y, z)$ at a plane $z = 0$, the angular spectrum is defined as the 2D Fourier transform:

$$ A(f_x, f_y; 0) = \mathcal{F}\{U(x, y, 0)\} = \int_{-\infty}^{\infty} \int_{-\infty}^{\infty} U(x, y, 0) \, e^{-j2\pi(f_x x + f_y y)} \, dx \, dy $$

where $f_x$ and $f_y$ are spatial frequencies (cycles per unit length).

Physical Interpretation

Each point $(f_x, f_y)$ in the angular spectrum represents a plane wave traveling in a specific direction. The spatial frequencies relate to propagation angles by:

$$ \sin\theta_x = \lambda f_x, \quad \sin\theta_y = \lambda f_y $$

where $\lambda$ is the wavelength and $\theta_x$, $\theta_y$ are the angles from the optical axis.

Spatial FrequencyPhysical Meaning
$(0, 0)$On-axis plane wave (straight through)
Large $f_x$ or $f_y$Steeply angled plane waves
$\sqrt{f_x^2 + f_y^2} > 1/\lambda$Evanescent waves (don’t propagate)

Propagation

The angular spectrum at a distance $z$ is:

$$ A(f_x, f_y; z) = A(f_x, f_y; 0) \cdot e^{j k_z z} $$

where the $z$-component of the wave vector is:

$$ k_z = \begin{cases} 2\pi\sqrt{\frac{1}{\lambda^2} - f_x^2 - f_y^2} & \text{if } f_x^2 + f_y^2 < \frac{1}{\lambda^2} \text{ (propagating)} \\ j2\pi\sqrt{f_x^2 + f_y^2 - \frac{1}{\lambda^2}} & \text{if } f_x^2 + f_y^2 > \frac{1}{\lambda^2} \text{ (evanescent)} \end{cases} $$

The field at any plane $z$ is obtained by inverse Fourier transform:

$$ U(x, y, z) = \mathcal{F}^{-1}\{A(f_x, f_y; z)\} $$

Advantages

  • Exact: No paraxial or Fresnel approximations required
  • Intuitive: Decomposes fields into plane wave components
  • Computational: Efficiently implemented via FFT algorithms
  • Unified: Handles both Fresnel and Fraunhofer regimes

Connection to Diffraction

For an aperture with transmission function $t(x, y)$ illuminated by a unit-amplitude plane wave:

$$ A(f_x, f_y) = \mathcal{F}\{t(x, y)\} $$

This directly gives the diffracted field’s angular distribution.

See Also