Rayleigh Effect

Rayleigh scattering, named after the British physicist Lord Rayleigh (John William Strutt),is the (dominantly) elastic scattering of light or other electromagnetic radiation by particles much smaller than the wavelength of the radiation.

The Main Idea

When light strikes small particles, it bounces off in a different direction in a process called scattering. Rayleigh scattering is the scattering that occurs when the particles are smaller than the wavelength of the light. This is the dispersion of electromagnetic radiation by particles that have a radius less than approximately 1/10 the wavelength of the radiation. The particles may be individual atoms or molecules. It can occur when light travels through transparent solids and liquids, but is most prominently seen in gases. Rayleigh scattering results from the electric polarizability of the particles. The oscillating electric field of a light wave acts on the charges within a particle, causing them to move at the same frequency. The particle therefore becomes a small radiating dipole whose radiation we see as scattered light.

A Mathematical Model

Lord Rayleigh calculated the scattered intensity from dipole scatterers much smaller than the wavelength to be:

[math]\displaystyle{ I = I_0 \frac{8\pi^4\alpha^2}{\lambda^4 R^2}(1+\cos^2\theta). }[/math]

I = resulting intensity of scattered light

I₀ = intensity of incident light

α = molecular polarizability

λ = wavelength of the light

θ = the scattering angle

Therefore, the intensity of the scattered light is inversely proportional to the fourth power of the wavelength of the incident light.

A Computational Model

How do we visualize or predict using this topic. Consider embedding some vpython code here Teach hands-on with GlowScript

Examples

The sun's light is a mix of violet, blues, greens through to reds. Blues and violets have the shortest wavelengths, that of blue is ~450 nanometres. Air molecules, mostly nitrogen and oxygen, are 1000X smaller still. They interact only very weakly with visible light but with their enormous numbers in the atmosphere the Rayleigh effect is clearly seen. Air molecules individually scatter sunlight it into all directions. Blue light is scattered much more strongly than longer wavelengths. The air above looks blue from that scattered sunlight. All other colors are scattered as well but progressively more weakly towards red. This is because the intensity of scattered light is inversely proportional to the fourth power of the wavelength of incident light and blue having the shortest wavelenth is scattered more, making the sky appear blue.

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