Linked from

The 25 pages that link to Mie scattering, each with the reason it gives.

• Interstellar dustRelated: Its size-dependent scattering helps determine how dust redirects visible and ultraviolet light.

• Interstellar extinctionRelated: Its wavelength-dependent scattering helps shape how dust removes light from a stellar beam.

• Weather radarRelated: Many raindrops scatter weather-radar wavelengths in this regime.

• Titanium dioxideRelated: Optimized pigment-particle sizes scatter visible light efficiently, producing opacity and whiteness.

• Structural colorationRelated: Microscopic particles can selectively scatter visible wavelengths and produce color.

• Transmission spectroscopyRelated: Cloud and haze particles can mute or reshape spectral features through Mie scattering.

• Zodiacal lightRelated: It describes how sunlight interacts with many zodiacal dust grains.

• Radar cross-sectionRelated: It provides exact sphere-scattering results that illustrate frequency-dependent RCS.

• VisibilityRelated: Aerosols and haze scatter visible light, often limiting sight distance.

• Bessel functionRelated: Its spherical-wave solutions use spherical Bessel functions.

• Atmospheric opticsRelated: It produces the whitish glare of clouds and haze that larger atmospheric particles create.

• Atmospheric extinctionRelated: Aerosols and dust produce this scattering, often adding nearly wavelength-independent dimming.

• Reflection nebulaRelated: Larger dust grains scatter light differently from the small-particle Rayleigh limit.

• GegenscheinRelated: It provides a framework for understanding sunlight scattered by dust-sized particles.

• Diffuse sky radiationRelated: Aerosols and droplets redirect sunlight across the sky, often producing brighter, less blue diffuse illumination.

• Kubelka–Munk equationRelated: Particle-level scattering can depart from the diffuse, two-flux simplification used to interpret S.