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.

• PolarizationRelated: Its angular pattern produces strongly polarized skylight away from the Sun.

• 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.

• Atmospheric perspectiveRelated: Scattered blue light contributes to the cool cast often seen in distant landscapes.

• Atmospheric windowRelated: It reduces transmission most strongly toward the blue and ultraviolet.

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

• PolarimetryRelated: Its polarization pattern helps explain polarized skylight and reveals scattering geometry.

• TwilightRelated: It redirects sunlight through the atmosphere after the Sun has set.

• Elastic scatteringBroader topic: It is a specific elastic process that explains wavelength-dependent scattering in gases.

• 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.

• Linear polarizationRelated: Scattered light can be strongly linearly polarized at particular viewing angles.

• Optical tweezersRelated: Its dipole approximation explains optical forces on particles far smaller than the laser wavelength.

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

• SunsetRelated: At sunset, sunlight travels farther through air, scattering more blue light out of the direct beam.

• Transmission spectroscopyRelated: A blueward slope in a spectrum can reveal scattering by small atmospheric particles.

• 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.

• Blue Ridge MountainsRelated: Atmospheric scattering contributes to the blue haze over the mountains.

• Light scatteringBroader topic: This small-particle regime explains why air preferentially scatters blue daylight.

• VisibilityRelated: Molecular scattering contributes to atmospheric extinction, especially along long sight lines.

• Solar radiationRelated: It redirects shorter-wavelength sunlight and contributes to the blue daytime sky.

• Atmospheric opticsRelated: It explains the blue daytime sky and the reddening of sunlight near the horizon.

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

• Atmospheric extinctionRelated: Air molecules scatter blue light more strongly, contributing to wavelength-dependent extinction.

• Blue eyesRelated: Shorter wavelengths scatter more strongly in the lightly pigmented iris, contributing to its blue appearance.

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

• Optical theoremBroader topic: In this limit, the theorem relates the dipole forward response to total scattered power.

• Pale Blue DotRelated: Scattered sunlight created the bright streak across which Earth appears.

• Optical isolatorRelated: Backscattered light in fibers can return toward a source that an isolator protects.

• Reflection nebulaRelated: It helps explain why reflection nebulae often look blue.

• Blue hourRelated: It helps explain why twilight skies can appear blue after direct sunlight fades.

• SunlightRelated: It scatters shorter-wavelength sunlight and helps make the daytime sky blue.

• Eye colorRelated: Scattering within the iris helps produce blue appearances despite little blue pigment.

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

• Belt of VenusRelated: It helps explain why the twilight sky glows red and pink.

• Diffuse sky radiationRelated: Air molecules scatter shorter wavelengths strongly, creating much of the blue diffuse light in a clear sky.

• HD 189733 bRelated: Scattering in the atmosphere contributes to the planet’s blue appearance.

• John William StruttBroader topic: His analysis explained why the clear sky appears blue.

• Sky blueRelated: It preferentially scatters blue sunlight through clear air, producing the color’s namesake appearance.