Rayleigh scattering

E179225

Rayleigh scattering is the physical phenomenon in which light or other electromagnetic radiation is elastically scattered by particles much smaller than its wavelength, explaining effects such as the blue color of the daytime sky.

All labels observed (1)

Label Occurrences
Rayleigh scattering canonical 3

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Statements (49)

Predicate Object
instanceOf light scattering mechanism
physical phenomenon
affects astronomical observations
optical communication through atmosphere
remote sensing measurements
appliesTo particles much smaller than the wavelength of radiation
causes partial polarization of skylight
contrastedWith Compton scattering
Mie scattering
Raman effect
surface form: Raman scattering
crossSectionDependsOn particle size to the sixth power for small particles
crossSectionProportionalTo 1/λ^4
dependsOn polarizability of scattering particles
refractive index fluctuations
energyChangeOfPhoton approximately zero
explains blue color of the daytime sky
bluish appearance of distant mountains
color of Earth's atmosphere when viewed from space
color of smoke and colloidal suspensions in some cases
reddish color of sunrise and sunset
firstDescribedBy Lord Rayleigh
surface form: John William Strutt, 3rd Baron Rayleigh
intensityProportionalTo 1/λ^4
isElastic true
isSubtypeOf coherent scattering
elastic scattering
lessEffectiveAt longer wavelengths
mathematicalDescriptionUses classical electromagnetic theory
dipole approximation
moreEffectiveAt shorter wavelengths
namedAfter Lord Rayleigh
occursFor molecules in air such as nitrogen and oxygen
occursIn Earth’s atmosphere
surface form: Earth's atmosphere

gases
liquids
planetary atmospheres
solids with small inhomogeneities
occursWhenParticleSizeIs much smaller than wavelength
relatedTo Mie theory
Tyndall effect
requiresCondition particle diameter much less than wavelength (d << λ)
scatters electromagnetic radiation
light
studiedIn astrophysics
atmospheric optics
climate science
optics
usedToCorrect atmospheric effects in satellite imagery
wavelengthDependence inversely proportional to the fourth power of wavelength
yearCharacterizedApprox 1871

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Referenced by (3)

Full triples — surface form annotated when it differs from this entity's canonical label.

Lord Rayleigh knownFor Rayleigh scattering