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Polarization Visualization

Interactive 2D and 3D demonstration of electromagnetic wave polarization. Explore how the amplitude ratio (ψ) and phase difference (δ) control linear, circular, and elliptical polarization patterns.

Use sliders to adjust parameters • Toggle 3D mode for spatial view
Ψ 45° Psi (Amplitude)
δ Delta (Phase)
📐 Linear Polarization
🎥 2D View Mode
📊 Wave Visualization
💡 How to Use

📚 Physics Background

🌊 Electromagnetic Wave Polarization

Polarization describes the orientation and behavior of the electric field vector in an electromagnetic wave. In a plane electromagnetic wave propagating through space, the electric field E⃗ and magnetic field B⃗ oscillate perpendicular to each other and to the direction of propagation (typically the z-axis).

This tool visualizes the electric field component, which traces out various shapes as the wave propagates—from straight lines (linear) to circles (circular) to ellipses (elliptical).

📐 Mathematical Formulation

For a wave propagating in the +z direction, the electric field components are given by:

Ex(z, t) = E0x cos(kz - ωt)

Ey(z, t) = E0y cos(kz - ωt + δ)

Where:

  • E0x and E0y are the amplitude magnitudes in the x and y directions
  • k = 2π/λ is the wave number (λ = wavelength)
  • ω = 2πf is the angular frequency (f = frequency)
  • δ is the phase difference between the x and y components
  • z is the position along the propagation direction
  • t is time

At a fixed point in space (e.g., z = 0), the electric field vector's tip traces an ellipse in the x-y plane as time progresses.

🎯 Parameters Explained

Ψ (Psi) - Amplitude Ratio Angle

The angle ψ relates to the ratio of amplitudes of the two perpendicular electric field components:

tan(ψ) = E0y / E0x

  • ψ = 0°: Only x-component (E0y = 0), horizontal linear polarization
  • ψ = 45°: Equal amplitudes (E0x = E0y), prerequisite for circular polarization
  • ψ = 90°: Only y-component (E0x = 0), vertical linear polarization

This parameter controls the shape of the polarization ellipse—specifically, how elongated or circular it is.

δ (Delta) - Phase Difference

The phase difference δ is the shift between the oscillations of the x and y components:

δ = φy - φx

  • δ = 0° or ±180°: Components oscillate in phase or exactly out of phase → Linear polarization
  • δ = +90°: y-component lags x-component by 90° → Right-hand circular (with ψ = 45°)
  • δ = -90°: y-component leads x-component by 90° → Left-hand circular (with ψ = 45°)
  • Other values: Create elliptical polarization with various orientations

This parameter controls the orientation and handedness of the polarization ellipse.

🔄 Polarization States and Physical Interpretation

🔸 Linear Polarization

Condition: δ = 0° or δ = ±180° (any ψ value)

Physical meaning: The electric field oscillates along a single direction in the x-y plane. The field vector traces a straight line as time evolves. The angle of this line with respect to the x-axis is determined by ψ.

When it occurs: Naturally from lasers, reflection off non-metallic surfaces at Brewster's angle, or transmission through polarizing filters (like polaroid sunglasses).

Applications: 3D cinema glasses, LCD displays, stress analysis, reducing glare.

⭕ Circular Polarization

Condition: ψ = 45° (equal amplitudes) AND δ = ±90°

Physical meaning: The electric field vector has constant magnitude but rotates uniformly in the x-y plane. The tip of the vector traces a circle. The direction of rotation determines handedness:

  • Right-hand (RH): δ = +90°, field rotates clockwise when viewed from the direction the wave is approaching
  • Left-hand (LH): δ = -90°, field rotates counter-clockwise

When it occurs: Passing linear polarized light through a quarter-wave plate at 45°, emission from certain astronomical sources, reflection from chiral molecules.

Applications: Satellite communications, radar systems, optical activity measurements, reducing signal degradation in fiber optics.

⬭ Elliptical Polarization

Condition: Any combination where δ ≠ 0°, ±90°, ±180° or ψ ≠ 45° with δ = ±90°

Physical meaning: The electric field vector traces an ellipse in the x-y plane. This is the most general case—linear and circular polarization are special cases of elliptical polarization. The ellipse has a specific orientation, aspect ratio (determined by ψ), and handedness (determined by sign of δ).

When it occurs: Most common in nature—partial reflection from surfaces, scattering in the atmosphere, propagation through birefringent crystals, or any system where phase and amplitude aren't perfectly controlled.

Applications: Ellipsometry (measuring thin film thickness and optical properties), polarimetry in astronomy and remote sensing, characterizing optical materials.

🔬 Related Optical Phenomena

Understanding polarization is essential for explaining various optical effects:

  • Brewster's Angle: At this specific angle of incidence, reflected light is perfectly linearly polarized perpendicular to the plane of incidence. Used in polarizing beam splitters and laser cavities.
  • Birefringence: In certain crystals (like calcite), light splits into two rays with different polarizations and velocities, creating double images. Used in wave plates and optical modulators.
  • Malus's Law: The intensity of light passing through a polarizer is I = I₀ cos²(θ), where θ is the angle between the light's polarization and the polarizer axis.
  • Faraday Effect: A magnetic field can rotate the plane of polarization—a magneto-optical effect used in optical isolators.
  • Photoelasticity: Mechanical stress induces birefringence in normally isotropic materials, revealing stress patterns with polarized light.

🌟 The Stokes Parameters

In advanced optics and astronomy, polarization is often described using the Stokes parameters (I, Q, U, V), which provide a complete description of the polarization state:

  • I: Total intensity
  • Q: Difference between horizontal and vertical linear polarization
  • U: Difference between +45° and -45° linear polarization
  • V: Difference between right and left circular polarization

The degree of polarization is P = √(Q² + U² + V²) / I, ranging from 0 (unpolarized) to 1 (fully polarized).