Linked from

The 44 pages that link to Rayleigh scattering, each with the reason it gives.

• Beer–Lambert lawCompared with: Scattered light can reduce transmission without being molecular absorption, complicating absorbance measurements.

• Raman spectroscopyCompared with: It is the intense, unshifted background from which Raman scattering must be separated.

• Compton scatteringCompared with: It changes photon direction without the Compton energy transfer.

• Interstellar extinctionCompared with: It offers a contrasting wavelength dependence to scattering by interstellar grains.

• Weather radarCompared with: It approximates echoes from small hydrometeors, unlike scattering by larger raindrops.

• Mie scatteringCompared with: It is the small-particle limit that Mie scattering extends beyond.

• Vibrational spectroscopyCompared with: Raman scattering is distinguished by its frequency shift from this elastic scattering.

• John TyndallCompared with: It explains blue skies through molecular scattering, unlike the infrared absorption central to Tyndall’s greenhouse research.

• Fresnel equationsCompared with: Unlike interface reflection, it redirects light through scattering within a medium.

• Thomson scatteringCompared with: Unlike Thomson scattering by a free charge, Rayleigh scattering involves bound charges and wavelength-dependent response.

• Diffuse reflectionCompared with: It redistributes light within a medium rather than describing rough-surface reflection.

• Thin-film interferenceCompared with: It can make blue-rich appearances without the paired reflections responsible for film colors.

• Atmospheric absorptionCompared with: It redirects radiation rather than transferring its energy through molecular absorption.

• C. V. RamanCompared with: It provides the unshifted background against which Raman-shifted light is detected.

• GegenscheinCompared with: The dust glow is not simply atmospheric Rayleigh scattering, which also brightens the sky.