Fourier Optics & Modern Diffraction Theory
2D Fourier transforms, convolution theorem, thin lens as an optical Fourier transformer, 4f spatial frequency filtering, and the Wiener-Khinchin theorem.
§7.1 Two-Dimensional Spatial Fourier Transforms and the Convolution Theorem
1. 2D Spatial Fourier Transform Pairs
Let $u(x, y)$ be the complex optical amplitude distribution in an aperture plane. Its two-dimensional Fourier transform $U(f_x, f_y)$ represents the spatial frequency spectrum of plane wave components: $$U(f_x, f_y) = \mathcal{F}\{u(x, y)\} = \int_{-\infty}^{\infty} \int_{-\infty}^{\infty} u(x, y) e^{-i 2\pi (f_x x + f_y y)} dx dy$$ where $f_x = \frac{k_x}{2\pi} = \frac{\sin \theta_x}{\lambda}$ and $f_y = \frac{k_y}{2\pi} = \frac{\sin \theta_y}{\lambda}$ are the spatial frequencies in cycles per unit length (e.g., $\text{lines/mm}$). The inverse Fourier transform reconstructs the original spatial distribution: $$u(x, y) = \mathcal{F}^{-1}\{U(f_x, f_y)\} = \int_{-\infty}^{\infty} \int_{-\infty}^{\infty} U(f_x, f_y) e^{i 2\pi (f_x x + f_y y)} df_x df_y$$2. Key Fourier Transform Theorems in Optics
- Linearity: $\mathcal{F}\{a u_1 + b u_2\} = a U_1 + b U_2$
- Spatial Scaling (Similarity): $\mathcal{F}\{u(ax, by)\} = \frac{1}{|ab|} U\left(\frac{f_x}{a}, \frac{f_y}{b}\right)$. Narrowing an aperture spatially spreads its diffracted spectrum in frequency space.
- Spatial Shift (Shift Theorem): $\mathcal{F}\{u(x - x_0, y - y_0)\} = U(f_x, f_y) e^{-i 2\pi (f_x x_0 + f_y y_0)}$
- Parseval’s Energy Theorem: $$\int_{-\infty}^{\infty} \int_{-\infty}^{\infty} |u(x, y)|^2 dx dy = \int_{-\infty}^{\infty} \int_{-\infty}^{\infty} |U(f_x, f_y)|^2 df_x df_y$$ Total optical radiant energy is conserved identically between the physical aperture plane and the spatial frequency Fourier plane.
3. The Convolution Theorem in Optical Imaging
The two-dimensional spatial convolution of an input object $g(x,y)$ with an optical system impulse response (point spread function) $h(x,y)$ is: $$g_{\text{out}}(x, y) = g_{\text{in}}(x, y) * h(x, y) = \int_{-\infty}^{\infty} \int_{-\infty}^{\infty} g_{\text{in}}(\xi, \eta) h(x - \xi, y - \eta) d\xi d\eta$$ The **Convolution Theorem** proves that convolution in space is mathematically equivalent to simple algebraic multiplication in frequency space: $$G_{\text{out}}(f_x, f_y) = G_{\text{in}}(f_x, f_y) \cdot H(f_x, f_y)$$ where $H(f_x, f_y) = \mathcal{F}\{h(x, y)\}$ is the **Optical Transfer Function (OTF)** of the imaging system.§7.2 The Thin Convex Lens as an Optical 2D Fourier Transformer
1. Phase Transformation of a Thin Lens
A thin spherical lens of focal length $f$ and refractive index $n$ possesses a variable glass thickness profile: $$\Delta(x, y) = \Delta_0 - \frac{x^2 + y^2}{2} \left( \frac{1}{R_1} - \frac{1}{R_2} \right) = \Delta_0 - \frac{x^2 + y^2}{2(n - 1)f}$$ When a plane wave traverses the lens, the spatially varying phase delay is: $$t_L(x, y) = e^{i k n \Delta(x,y)} e^{i k [\Delta_0 - \Delta(x,y)]} = e^{i k \Delta_0} \exp\left[ -i \frac{k}{2f} (x^2 + y^2) \right]$$ Dropping the constant phase factor $e^{i k \Delta_0}$, the **lens transmission function** is: $$t_L(x, y) = \exp\left[ -i \frac{k}{2f} (x^2 + y^2) \right]$$2. Field in the Back Focal Plane
Place an input transparency with optical field distribution $u_0(x, y)$ in the front focal plane of the lens ($z = -f$). Applying the Fresnel diffraction integral from the input plane to the lens, multiplying by the lens transmission function $t_L(x, y)$, and propagating to the back focal plane ($z = +f$): The quadratic phase factors cancel completely, leaving: $$u_f(u, v) = \frac{1}{i \lambda f} \int_{-\infty}^{\infty} \int_{-\infty}^{\infty} u_0(x, y) \exp\left[ -i \frac{2\pi}{\lambda f} (u x + v y) \right] dx dy$$ This is the exact mathematical Fourier transform of the input object $u_0(x, y)$ evaluated at spatial frequencies: $$f_x = \frac{u}{\lambda f}, \quad f_y = \frac{v}{\lambda f}$$ Every spatial coordinate $(u, v)$ in the back focal plane corresponds to a specific spatial frequency of the input image.§7.3 Spatial Frequency Filtering in the 4f Correlator and the Wiener-Khinchin Theorem
1. Architecture of the 4f System
The 4f system consists of two identical lenses $L_1$ and $L_2$ of focal length $f$ separated by distance $2f$:- Input Plane $P_1$ ($z = 0$): Object transparency $u_{\text{in}}(x, y)$.
- Fourier Plane $P_2$ ($z = 2f$): Lens $L_1$ forms the optical Fourier transform $U(f_x, f_y)$. A physical spatial filter (mask) $H(f_x, f_y)$ is inserted here.
- Output Plane $P_3$ ($z = 4f$): Lens $L_2$ takes the inverse Fourier transform, synthesizing the filtered output image: $$u_{\text{out}}(x, y) = \mathcal{F}^{-1} \{ U(f_x, f_y) \cdot H(f_x, f_y) \}$$
2. Types of Optical Spatial Filters
- Low-Pass Filter (Circular Pinhole Mask): Blocks high spatial frequencies ($f_r > f_c$). Removes high-frequency noise, speckle, and grain, producing a smooth image.
- High-Pass Filter (Opaque Central Dot): Blocks the zero-order DC frequency ($f_x = f_y = 0$). Highlights sharp edges, boundaries, and high-frequency textural details while suppressing uniform background illumination.
- Directional Filter (Slit Mask): Eliminates periodic grating lines oriented along specific angles (e.g., removing raster scanning lines from video images).
3. The Wiener-Khinchin Theorem in Optical Coherence
The mutual coherence function (autocorrelation) of an optical field $\Gamma(\tau)$ is: $$\Gamma(\tau) = \langle E^*(t) E(t + \tau) \rangle = \lim_{T \to \infty} \frac{1}{2T} \int_{-T}^T E^*(t) E(t + \tau) dt$$ The **Wiener-Khinchin Theorem** establishes that the power spectral density $S(\nu)$ of an optical field is the Fourier transform of its temporal autocorrelation function $\Gamma(\tau)$: $$S(\nu) = \int_{-\infty}^{\infty} \Gamma(\tau) e^{-i 2\pi \nu \tau} d\tau$$ $$\Gamma(\tau) = \int_{-\infty}^{\infty} S(\nu) e^{i 2\pi \nu \tau} d\nu$$ This theorem is the physical foundation of Fourier Transform Spectroscopy (FTS), where the emission spectrum of a star or chemical compound is recovered by Fourier transforming the interferogram measured by a Michelson interferometer.📝 Chapter Worked Examples & Exercises
Complete derivations & analytical proofsA 4f optical spatial filtering system uses a laser of wavelength $\lambda = 632.8 ext{ nm}$ and two lenses of focal length $f = 250 ext{ mm}$. The input object is a photograph corrupted by high-frequency periodic grid noise with spatial frequency $f_{ ext{noise}} = 50.0 ext{ lines/mm}$. (a) Calculate the radial position $r_{ ext{noise}}$ of the noise spectral peaks in the Fourier transform plane. (b) What maximum pinhole aperture diameter $D_{ ext{filter}}$ should be placed in the Fourier plane to completely eliminate the grid noise while retaining image content up to $40.0 ext{ lines/mm}$?
The noise components appear as bright diffraction spots at radius $7.91 ext{ mm}$ from the optical axis.
The desired image frequencies extend out to radius $6.33 ext{ mm}$.
A pinhole diameter of $14.0 ext{ mm}$ transmits all signal up to $40 ext{ lines/mm}$ while completely blocking the $50 ext{ lines/mm}$ noise.