Linked from
The 39 pages that link to Albedo, each with the reason it gives.
Radiative forcingRelated: Albedo changes alter how much solar energy Earth absorbs.
Rayleigh scatteringRelated: Scattering by atmospheres and particles helps determine how much radiation is reflected.
ReforestationRelated: Dark forests can absorb more sunlight than the open land they replace, affecting local climate.
Solar irradianceRelated: Together with irradiance, albedo determines how much solar energy a surface absorbs.
ClimateRelated: Changes in snow, ice, clouds, or land cover alter how much solar energy Earth absorbs.
SeasonsRelated: Snow and ice reflect sunlight, reinforcing seasonal cooling in some regions.
AfforestationRelated: Darker tree cover can reduce surface reflectivity and partly offset climate cooling.
MicroclimateRelated: Differences in surface reflectivity change how much solar energy a place absorbs.
Greenland ice sheetRelated: Snow and clean ice reflect sunlight, while darker surfaces absorb more energy and melt faster.
SnowmeltRelated: Fresh, bright snow reflects much sunlight, while darker or dirty snow absorbs more energy.
IceRelated: Bright ice reflects sunlight and helps regulate how much energy Earth absorbs.
SnowpackRelated: Bright snow reflects much sunlight, while darkening increases absorbed energy and can speed melt.
Ice ageRelated: Expanding bright ice reflects sunlight and reinforces cooling, while retreating ice weakens that feedback.
Climate of the ArcticRelated: Bright snow and ice reflect sunlight, while darker ocean absorbs more energy.
GlaciationRelated: Bright snow and ice reflect sunlight, reinforcing cooling and ice growth.
Faint young Sun paradoxRelated: A darker early Earth would have absorbed more sunlight despite the Sun’s lower luminosity.
Polar climateRelated: Snow and ice reflect much sunlight, limiting surface warming.
Climate change and forestsRelated: Forests can absorb more sunlight than snow-covered land, complicating their cooling effect.
James LovelockRelated: Daisyworld’s contrasting daisies change planetary albedo and thereby influence temperature.
Huronian glaciationRelated: Expanding ice reflects more sunlight, creating a positive feedback that can intensify cooling.
Reflection nebulaRelated: Dust albedo helps set how much nearby starlight can emerge as scattered light.
Sturtian glaciationRelated: Expanding ice increased reflectivity, reinforcing cooling as glaciation spread.
SunlightRelated: Albedo determines how much incoming sunlight warms a surface.
HaptophyteRelated: Coccolithophore blooms can increase ocean-surface reflectance through suspended calcite plates.
Marinoan glaciationRelated: Expanding ice raised planetary reflectivity, reinforcing cooling in Snowball Earth models.
Earth’s shadowRelated: The Moon’s reflectivity affects how bright it appears against Earth’s dark shadow.
Black (color)Related: Low visible-light albedo is characteristic of surfaces perceived as black.
Deforestation and climate changeRelated: Forest removal changes surface reflectivity, which can partly offset or amplify local warming.
Mikhail BudykoRelated: Snow and ice reflect sunlight, linking Budyko’s heat balance to powerful climate feedback.