ANTHILLAsk your own question
Nature and Space · 5 min read · full version

Blue Sky, Gray Day: What the Evidence Really Shows

Simultaneous cyanometer readings taken at Geneva and from a mountain summit differed by altitude: Geneva registered a whiter shade, about 7, while the summit read a dark blue of 1 to 2 20.

Internet Archive See source for rights
Last checked 2026-10-21. Sentence check: 7 paragraphs passed, 8 repaired, 2 removed. Every number links to the exact quote. Read the easy version

In short

The checked evidence says Rayleigh scattering by air molecules is responsible for the blue color of the sky under clear conditions 59, and that air molecules favor blue light, producing the deep blue sky 60. Rayleigh scattering applies to particles much smaller than the wavelength of light 14. Larger particles behave differently: tropospheric aerosols, such as smoke particles, scatter with a much weaker wavelength dependence, so they add more evenly colored light that dilutes the blue 62. Near the horizon, the light has passed through more air and through dusty, humid layers near the ground, and Mie scattering and repeated Rayleigh scattering wash the blue out toward white 78. Smoke is one such aerosol. In July 2026, Canadian wildfires carried smoke and hazardous air to Chicago, Minneapolis, and New York City 2, but that report does not address sky color. The checked evidence does not describe conditions in October 2026, so it cannot tell us which factor is making a particular sky look paler today.

A gauge for blue, in the 1700s

Horace-Bénédict de Saussure invented the cyanometer, a simple gauge with 52 hues of blue arranged from light to dark on a graded circular scale, to measure how blue the sky is 17. The scale ran in equal steps from white through blue (Prussian blue) to black 21.

Saussure held that the sky's azure depended on the amount of opaque vapors in the atmosphere linked to meteorological phenomena 22. Later, Rayleigh proposed that pure air alone, without colloidal particles, causes the scattering that makes the sky blue 76.

The gauge also showed that the sky's color changes with height. Simultaneous readings differed by altitude: a whiter shade of 7 at Geneva versus a dark blue of 1–2 from the summit 2019.

Pure air and the opponent idea, 1870s to 1901

Ewald Hering proposed three opponent color pairs (blue–yellow, red–green, black–white) as separate chemical processes in the retina 44. His opponent-color idea was developed before cone receptors or cone photopigments were known 4.

Lord Rayleigh gave an explanation for the blue color of the sky as part of his work in optics 61, and in 1899 he proposed that pure air alone causes the scattering 76. Rayleigh scattering is defined as scattering by particles much smaller than the wavelength of light 14. A different effect, the Tyndall effect, makes a medium look whitish and turbid when the particles are larger than the wavelength of light 71, but the Tyndall effect itself is not responsible for the blue color of the sky 73.

In 1901, Pernter published a study on the polarization of light in turbid media and of skylight, aimed at explaining the blue color of the sky 38. He also took polarization measurements alongside scintillation observations 41.

Eyes and brains: turning light into blue

Three cone types, sensitive to blue, green, and red, send signals to color-opponent ganglion cells in the retina 4748. At the neural level, red and green signals are subtracted to form a red-green channel, while their addition produces a yellow signal that is subtracted from the blue signal in the yellow-blue channel 51. Neurophysiological research has confirmed that Hering's three opponent processes actually exist, though his ideas were highly simplified 54.

The eye also adjusts to its surroundings. Sensitivity changes beginning at the first stages of visual transduction let neurons with a modest dynamic range respond to contrast across a huge range of mean illumination 31. Background light can reduce photoreceptor sensitivity even when it bleaches almost none of the photopigment, which is one way a bright surround can make a dim target harder to see 32. Rods lose their voltage response entirely (saturate) once roughly 12% of their rod pigment has been bleached 36.

People also differ. Individual cone sensitivities can be inferred from each person's color matching functions, implying that observers' cone responses can differ 5. Older observers showed more variability between individuals in color matching 9, and standard CIE parameters may not apply to these observers 12.

When the air gets busy: haze, humidity and smoke

Air molecules and larger particles scatter light in very different ways. Tropospheric aerosols such as smoke particles scatter with a much weaker wavelength dependence than air molecules, so they add more evenly colored light that dilutes the blue 62. Mie scattering, from particles similar in size to light's wavelength such as water droplets, dust, and pollution, scatters all visible wavelengths more evenly, producing a whiter, washed-out appearance 77. As haze thickens, the B/R ratio of the sky falls toward 1.0 and the sky shifts from blue to gray 63.

Humidity matters too. Visibility drops sharply once humidity rises above 80%, even if the number of pollutant particles stays the same 16. Fine particles are particularly important for total optical extinction because they scatter light efficiently 64. During haze, the aerosol scattering coefficient rose to about 0.665 per km, versus about 0.213 per km on non-haze days, showing that scattering makes up most of the light extinction 69.

Looking at the horizon makes this worse. Above the observer there is about 8 miles of atmosphere, while the light reaching the eye from the horizon has traveled through 100 miles or more 74. Near the horizon, Mie scattering and repeated Rayleigh scattering wash the blue out toward white 78.

Where things stand now (October 2026)

Near the horizon, light travels through more air and particle-filled layers, so extra Mie scattering from dust and pollution adds white light and makes the blue look paler 7275. Smoke and cloud signals overlap in attenuated backscatter color ratio, which causes the algorithm to misclassify some smoke plumes as clouds 29.

Still unknown

The checked evidence gives Rayleigh scattering's preference for blue but not the exact wavelength law that sets its strength, and the violet-versus-blue puzzle (why the sky is blue rather than violet) appears in the research notes but has no numbered evidence; these two lanes are thin in what can be cited.

No checked source describes sky conditions in October 2026. The newest checked evidence is from July 2026, so how smoke, humidity, or haze are affecting skies right now is an open question.

How much each factor (smoke dilution, humidity, horizon path length) contributes to a particular pale or gray sky is not quantified in the checked evidence, and the aerosol threshold at which the sky shifts from blue to white remains unsettled.

Explore this colony and ask your own questions

Connected to other stories

Canada also appears in How did the Federal Reserve Act change who could create money?, How early did people really reach Australia and Asia?, Where did Cajun and Creole people really come from?, What are the best ways to make money online in 2027?, Is the US government really poisoning us with processed food?, How long has AI been around for everyone to use?, Could One Bitcoin Really Be Worth $200,000?, How much would 10 sales a day at $500 make?, Can you really make money trading crypto?, Who Is the Richest Freemason, and Can We Prove It?, Can Anyone Really Name the First Horror Movie Ever Made?.

Albert Einstein also appears in Is it really only three licks to reach a Tootsie Pop center?, Has Anyone Ever Used the Internet for Time Travel?, If Earth spins so fast, why don't spacecraft get left behind?.

Australia also appears in How did the Federal Reserve Act change who could create money?, How early did people really reach Australia and Asia?, Is the US government really poisoning us with processed food?, How long has AI been around for everyone to use?, Can you really make money trading crypto?, What was the first real crypto trade, and when did it happen?, Can Anyone Really Name the First Horror Movie Ever Made?.

NASA also appears in If Earth spins so fast, why don't spacecraft get left behind?, Why hasn't anyone flown to Mars yet?.

Sun also appears in Has Anyone Ever Used the Internet for Time Travel?, If Earth spins so fast, why don't spacecraft get left behind?, Why hasn't anyone flown to Mars yet?.

Earth also appears in If Earth spins so fast, why don't spacecraft get left behind?, Why hasn't anyone flown to Mars yet?.

New England also appears in Where did Cajun and Creole people really come from?.

Quebec also appears in How did the Federal Reserve Act change who could create money?.

Sources

[1] supported · established source
The smoke has left city skies gloomy, though daily life continued under them.
"Yet, as photos show, daily life continued under gloomy skies."
Photos Show Wildfire Smoke Engulfing Cities Across the U.S. and Canada · saved copy
[2] supported · established source
Wildfires raging in Canada have carried smoke and hazardous air to Chicago, Minneapolis, New York City and other cities.
"Wildfires raging in Canada have spread smoke and hazardous air to Chicago, Minneapolis, New York City and beyond."
Photos Show Wildfire Smoke Engulfing Cities Across the U.S. and Canada · saved copy
[3] supported · established source
Officials issued hazardous air quality alerts and health warnings, advising sensitive groups such as children and people with asthma to limit time outdoors.
"Officials are advising sensitive groups, including children and people with asthma, to limit their time outdoors."
Photos Show Wildfire Smoke Engulfing Cities Across the U.S. and Canada · saved copy
[4] documented · scholarly source
The opponent-process idea of color perception was developed by E. Hering before cone receptors or cone photopigments were known.
"The idea of opponent or antagonistic processes as the basic physiological substrate of our ability to perceive colors was originally developed by E. Hering before the discovery of what was initially called visual purple, and long before anything at all was known about cone receptors or the cone photopigments."
Opponent-Colours Theory in the Light of Physiological Findings (1985)
[5] supported · scholarly source
Individual cone sensitivities can be inferred from each person's individual color matching functions, which is a classic problem in color vision, implying that observers' cone responses can differ.
"Estimating individual cone sensitivities on the basis of their corresponding individual color matching functions is a classic problem of color vision."
Estimation of an individual's Human Cone Fundamentals from their Color Matching Functions (2010)
[6] documented · scholarly source
The study found that the chromaticity domain enclosed by the spectrum locus and purple line does not contain the chromaticity coordinates of all stimuli, and spectral chromaticity coordinates do not follow wavelength order along the spectrum locus.
"It is found that the domain 𝛺 does not contain the chromaticity coordinates of all stimuli, and spectral chromaticity coordinates do not distribute in the wavelength order along the spectrum locus, which results in no way to determine the Helmholtz coordinates for certain stimuli."
CIE Colour Matching Functions and Cone Fundamentals: Problems and Modifications (2024)
[7] supported · scholarly source
Hering believed the antagonistic color mechanisms were neural and linked to opposite neurochemical processes.
"Hering’s antagonistic mechanisms were thought by him to be neural, and to be somehow associated with opposite neurochemical processes."
Opponent-Colours Theory in the Light of Physiological Findings (1985)
[8] supported · scholarly source
It was previously assumed that the chromaticity diagrams based on the CIE 1931 or 1964 colour matching functions contained all possible chromaticity coordinates of stimuli.
"In the past it was generally accepted that the chromaticity diagram based on either 1931 or 1964 colour matching functions (CMFs), contains all the chromaticity coordinates of stimuli"
CIE Colour Matching Functions and Cone Fundamentals: Problems and Modifications (2024)
[9] supported · scholarly source
Older observers showed more variability between individuals in colour matching, which helps explain why two people can match the same colour differently.
"The experimental results show relatively little variability with age, except as expected increases in lens density with age, and older observers showed more inter-observer variability."
The Age Effect on Observer Colour Matching and Individual Colour Matching Functions (2023)
[10] supported · scholarly source
Hering published quantitative studies of metameric color mixture and considered effects such as intensity invariance of color matches and the influence of macular pigment.
"although he published quantitative studies of metameric color-mixture and was concerned with matters such as intensity invariance of color matches and the influence of macular pigment on such data"
Opponent-Colours Theory in the Light of Physiological Findings (1985)
[11] supported · scholarly source
Individual observers' color matching data are tested under the assumption that they share a common photopigment spectral absorptance, the Stockman and Sharpe 10 degree function.
"with the assumption that they have the Stockman and Sharpe 10 degree photo-pigment spectral absorbtance in common."
Estimation of an individual's Human Cone Fundamentals from their Color Matching Functions (2010)
[12] supported · scholarly source
Standard mean colour matching parameters assumed by the CIE, such as macular pigment optical density, may not apply to these observers, indicating that individual differences matter.
"The analysis suggests that some of the mean colour matching parameters assumed by the CIE, such as the macular pigment optical density, do not apply for these observers."
The Age Effect on Observer Colour Matching and Individual Colour Matching Functions (2023)
[13] supported · reference source
Mie theory explains the scattering of any spherical particle regardless of its size parameter.
"La dispersión de cualquier partícula esférica con un parámetro de tamaño arbitrario se explica por la teoría de Mie ."
Translation: The scattering of any spherical particle with an arbitrary size parameter is explained by Mie theory.
Dispersión de la luz por partículas
[14] supported · reference source
Rayleigh scattering is defined as scattering by particles much smaller than the wavelength of light, in the small size-parameter regime.
"La dispersión de Rayleigh se puede definir como la dispersión en un régimen de parámetros de tamaño pequeño X<<1 ."
Translation: Rayleigh scattering can be defined as scattering in a regime of small size parameters X<<1.
Dispersión de la luz por partículas
[15] supported · reference source
Multiple scattering effects from particles are treated with radiative transfer techniques.
"Los efectos de dispersión múltiple de la dispersión de la luz por las partículas se tratan mediante técnicas de transferencia radiativa"
Translation: The multiple scattering effects of light scattering by particles are treated using radiative transfer techniques.
Dispersión de la luz por partículas
[16] supported · niche source
Visibility drops sharply once humidity rises above 80%, even if the number of pollutant particles stays the same.
"Above 80%, it becomes rapid, and visibility drops sharply even if the actual number of pollutant particles in the air hasn't changed."
Why Is There a Haze in the Air Today? Main Causes - ScienceInsights · saved copy
[17] supported · niche source
Horace-Bénédict de Saussure invented the cyanometer, a simple gauge with 52 hues of blue arranged from light to dark on a graded circular scale, to measure how blue the sky is.
"He invented a rather simple gage that consisted of 52 different hues of blue arranged from light to dark on a gradated circular scale."
Cyanometer — Colour Studies
[18] documented · scholarly source
The cyanometer was a simply constructed measuring instrument used to determine the blueness of the sky.
"The cyanometer is a simply constructed measuring instrument that enables a determination of skyblue."
Himmelblau – das Cyanometer des <i>Horace-Bénédict de Saussure</i> (1740–1799) (2011)
[19] supported · niche source
The cyanometer helped confirm that the colour of the sky changes with elevation.
"His device, called a cyanometer, helped to confirm that the sky’s colour changed with the elevation."
Cyanometer — Colour Studies
[20] supported · scholarly source
Simultaneous cyanometer readings differed by altitude: a whiter shade of 7 at Geneva versus a dark blue of 1–2 from the summit.
"Simultaneous measurements gave a whiter shade of 7 at Geneva but a dark blue of 1–2 from the summit."
Sixteen shades of blue; the use of a digital camera as a cyanometer (2026)
[21] documented · scholarly source
The cyanometer consisted of a circular color scale running in equal steps from white through blue (Prussian blue) to black.
"It consists of a color-scale that is arranged circularly going in equal steps from white to blue (Prussian blue) and finally into black."
Himmelblau – das Cyanometer des <i>Horace-Bénédict de Saussure</i> (1740–1799) (2011)
[22] documented · scholarly source
Its inventor, Horace-Bénédict de Saussure, held that the sky's azure depended on the amount of opaque vapors in the atmosphere linked to meteorological phenomena.
"According to its inventor - Horace-Bénédict de Saussure - the azure is determined by the amount of so called opaque vapors in the atmosphere associated with meteorological phenomena."
Himmelblau – das Cyanometer des <i>Horace-Bénédict de Saussure</i> (1740–1799) (2011)
[23] supported · scholarly source
The document attributes a secondary red/green maximum in volcanic twilights, seen at sun depressions greater than 6°, to multiple scattering rather than mesospheric dust. It does not give a quantitative share of the glow from multiply scattered light.
"This seems to have been caused by multiple scattering and not by mesospheric dust."
Twilights and Stratospheric Dust Before and After the Agung Eruption (1969)
[24] documented · scholarly source
The paper reports that multiple scattering has relatively minor influence on recovering stratospheric dust properties from twilight sky measurements, provided the mean altitude of the haze layer is between 10 and 30 km. The document gives no specific percentage for the share of multiply scattered light.
"The presence of haze in the lower troposphere and the occurrence of multiple scattering both have relatively minor influences on the recovery of the stratospheric dust properties, provided that 10< \(\overline h \) <30 km."
Radiance and color of the sky at twilight: Perturbations caused by stratospheric haze (1980)
[25] documented · scholarly source
Near-horizon illumination on Titan is strongest when the Sun is highest in the sky, which the authors attribute to the intensity of multiple scattering.
"The total near-horizon illumination maximizes when the Sun is highest in the sky owing to the intensity of multiple scattering."
Titan’s Twilight and Sunset Solar Illumination (2018)
[26] supported · scholarly source
Light reaching the surface from low in the sky near Titan's horizon is diffusely scattered light.
"Shadows below the lander should receive illumination from diffusely scattered light low in the sky near Titan's horizon."
Titan’s Twilight and Sunset Solar Illumination (2018)
[27] supported · scholarly source
In the twilight solar zenith angle range of 88–94°, single scattering plays a dominant role in the sky brightness, while the relative contribution of multiple scattering depends on the aerosol loading.
"showsthatsinglescatteringplaysadominantroleintheSZA"
Nabro volcano aerosol in the stratosphere over Georgia, South Caucasus from ground-based spectrometry of twilight sky brightness (2013)
[28] supported · scholarly source
The CALIOP Cloud and Aerosol Discrimination algorithm separates clouds from aerosols using multidimensional probability density functions built from a large training set of CALIOP measurements.
"clouds are distinguished from aerosols using multidimensional probability density functions derived from an extensive training set of CALIOP measurements"
GMD - TRAILS
[29] supported · scholarly source
Smoke and cloud signals overlap in attenuated backscatter color ratio, which causes the algorithm to misclassify some smoke plumes as clouds.
"This arises from overlapping attenuated backscatter color ratios (0.5–0.9)"
GMD - TRAILS
[30] supported · scholarly source
The depolarization criterion is adjusted to account for cirrus clouds, which have high depolarization because their ice crystals are non-spherical.
"This accounts for cirrus clouds' high depolarization (from non-spherical ice crystals)."
GMD - TRAILS
[31] supported · scholarly source
Sensitivity changes beginning at the first stages of visual transduction let neurons with a modest dynamic range respond to contrast across a huge range of mean illumination, which is the basis for adapting to bright or dim surroundings.
"Sensitivity changes, beginning at the first stages of visual transduction, permit neurons with modest dynamic range to respond to contrast variations across an enormous range of mean illumination."
Chromatic Light Adaptation Measured using Functional Magnetic Resonance Imaging (2002)
[32] documented · scholarly source
Background light can reduce photoreceptor sensitivity even when it bleaches almost none of the photopigment, which is one way a bright surround can make a dim target harder to see.
"Background fields which bleached less than 0.5% rod pigment nevertheless diminished photoreceptor sensitivity."
Action Spectra and Adaptation Properties of Carp Photoreceptors (1973)
[33] documented · scholarly source
Adaptation of a probe's signal depends on the mean light absorption in the same cone class: backgrounds that change absorption in the L and M cones affect L and M cone-initiated signals, but backgrounds seen only by S cones do not.
"We found that signals from probes initiated in the L and M cones were affected by backgrounds that changed the mean absorption rates in the L and M cones, but not by background changes seen only by the S cones."
Chromatic Light Adaptation Measured using Functional Magnetic Resonance Imaging (2002)
[34] supported · scholarly source
How quickly receptor sensitivity recovers after exposure to a background field depends on the total light flux (intensity multiplied by time) of that field.
"The degree and rate of recovery of receptor sensitivity after exposure to a background field was a function of the total flux (I x t) of the field."
Action Spectra and Adaptation Properties of Carp Photoreceptors (1973)
[35] documented · scholarly source
The measured fMRI signals are consistent with a simple mean-field adaptation model based on Naka-Rushton adaptation mechanisms operating within each cone photoreceptor class.
"show that the quantitative fMRI signals are consistent with a simple model of mean-field adaptation based on Naka-Rushton (Naka and Rushton, 1966) adaptation mechanisms within cone photoreceptor classes."
Chromatic Light Adaptation Measured using Functional Magnetic Resonance Imaging (2002)
[36] supported · scholarly source
Rods lose their voltage response entirely (saturate) once roughly 12% of their rod pigment has been bleached.
"Rod saturation, i.e. the abolition of rod voltages, occurred after approximately 12% of rod pigment was bleached."
Action Spectra and Adaptation Properties of Carp Photoreceptors (1973)
[37] documented · scholarly source
The study found that the degree of polarization is a key parameter indicating how accurate angle-of-polarization measurements of skylight are.
"The results of experiments reveal that the DOP is a key parameter to indicate the accuracy of AOP measurements, and all the output solar meridian orientations extracted by our method in both clear and cloudy skies can achieve a high accuracy for vehicle orientation."
An Evaluation of Skylight Polarization Patterns for Navigation (2015)
[38] supported · reference source
Pernter published a 1901 study on the polarization of light in turbid media and of skylight, aimed at explaining the blue color of the sky.
"1901: Untersuchungen über die Polarisation des Lichtes in trüben Medien und des Himmelslichtes mit Rücksicht auf die Erklärung der blauen Farbe des Himmels"
Translation: 1901: Investigations on the polarization of light in turbid media and of skylight, with regard to explaining the blue color of the sky
Josef Maria Pernter
[39] supported · niche source
The skylight polarization pattern arises from scattering of sunlight in the atmosphere and is modeled from Rayleigh scattering theory combined with solar position.
"Model and prediction of skylight polarization distribution pattern that arises due to scattering of sunlight in the atmosphere plays a vital role in bionic navigation sensor system."
Simulation and Prediction for Rayleigh Skylight Polarization Distribution (2007)
[40] supported · reference source
The polarization pattern of skylight that depends on the sun's position is not visible to humans.
"Durch Streulicht am blauen Himmel entsteht ein für den Menschen nicht sichtbares charakteristisches Muster teilweise polarisierten Lichts, das vom Stand der Sonne abhängig ist."
Translation: Scattered light from the blue sky produces a characteristic pattern of partially polarized light that is not visible to humans and depends on the position of the sun.
Karl von Frisch
[41] supported · reference source
Pernter took measurements of the polarization of skylight, alongside scintillation observations.
"Ebenso nahm er Messungen der Polarisation des Himmelslichtes und Szintillationsbeobachtungen vor"
Translation: Likewise, he carried out measurements of the polarization of skylight and scintillation observations.
Josef Maria Pernter
[42] supported · niche source
Insects such as flies, honeybees, and desert ants can see the polarization pattern of the sky and use it for navigation, unlike humans.
"However, insects e.g. flies, honeybees, desert ants, will be able to see the polarization signature of the sky anduseitfornavigation."
PDF e.g. i.e. - bpb-us-e2.wpmucdn.com
[43] supported · niche source
The polarimetric signal of scattered light depends on the angle of the incoming sunlight, which is why the sun's position shapes the polarization pattern.
"polarimetric signal is also dependent on the incident angle of the sunlight [3]."
PDF e.g. i.e. - bpb-us-e2.wpmucdn.com
[44] supported · reference source
Hering proposed three opponent color pairs (blue–yellow, red–green, black–white) as separate chemical processes in the retina, each with an inhibiting and an exciting part.
"Darum vermutete er drei getrennte chemische Prozesse in der Netzhaut mit je zwei Gegenfarben , mit je einem hemmenden und einem erregenden Anteil, die nach einem Gleichgewicht streben."
Gegenfarbtheorie
[45] supported · niche source
A normal trichromat needs three primary colors (red, blue, and green) to match all other colors, which reflects the three cone types the eye uses.
"Initially, the normal trichromat is the type in which three colors are required to equal all the other colors: red, blue, and green (Matlin and Foley 1996)."
Color and shape perception in people with color blindness (2026)
[46] supported · niche source
The same set of photoreceptors can produce different visual outputs depending on the retinal circuitry that processes their signals, so opsin genes alone cannot predict what an animal perceives.
"the same photoreceptor repertoire can potentially generate different visual outputs depending on retinal circuitry"
Guppy color vision: opsin diversity, retinal physiology, plasticity, and evolutionary significance (2026)
[47] supported · reference source
Three cone types with peak sensitivity to short (blue), medium (green) and long (red) wavelengths send signals to color-opponent ganglion cells in the retina.
"Drei verschiedene Zapfentypen im Auge, die jeweils ihre höchste Empfindlichkeit für kurz (blau)-, mittel (grün)- und langwelliges (rot) Licht haben, liefern Signale an die nachgeschalteten farbopponenten Ganglienzellen der Netzhaut (neuronale Farbkanäle)."
Gegenfarbtheorie
[48] supported · reference source
The three cone types are sensitive to blue (S-cones), green (M-cones) and red (L-cones), and this is the physiological basis of color vision.
"Die Ursache liegt in den drei Zapfen des Farbsehens. Diese haben ihre Empfindlichkeiten für Blau (S-Zapfen), Grün (M-Zapfen) und Rot (L-Zapfen)."
Translation: The cause lies in the three cones of color vision. These have their sensitivities for blue (S-cones), green (M-cones) and red (L-cones).
Kries-Zonentheorie
[49] supported · niche source
Color blindness arises when one or more of the three cone types is deficient, which makes color perception difficult and lowers color contrast.
"since with color blindness, the deficit of one or more of the three cones makes color perception difficult, which makes color contrast low."
Color and shape perception in people with color blindness (2026)
[50] supported · niche source
Horizontal cells pool signals from neighboring photoreceptors and feed back onto photoreceptor synaptic terminals, contributing to spatial and spectral integration.
"Horizontal cells contribute substantially to spatial and spectral integration by pooling signals from neighboring photoreceptors and providing feedback to the photoreceptor synaptic terminals"
Guppy color vision: opsin diversity, retinal physiology, plasticity, and evolutionary significance (2026)
[51] supported · reference source
At the neural level, red and green signals are subtracted to form a red-green channel, while their addition produces a yellow signal that is subtracted from the blue signal in the yellow-blue channel.
"Auf der neuronalen Ebene werden die Zapfensignale „verschaltet“: „Rot“ und „Grün“ werden subtrahiert, die Differenz wird im Rot-Grün-Kanal weitergeleitet; die Addition von „Rot“ und „Grün“ dagegen ergibt ein Signal, dem die Empfindung von Gelb entspricht; diese Signale werden vom „Blau“-Signal subtrahiert und im Gelb-Blau-Kanal weitergeleitet."
Gegenfarbtheorie
[52] supported · reference source
Johannes von Kries combined the three-component theory with the opponent-color theory by dividing color vision into a peripheral zone and a central zone.
"Um diesen Konflikt von drei oder vier Grundfarben zu entschärfen, teilte Kries den Vorgang des Farbensehens in eine periphere und eine zentrale Zone."
Translation: To defuse this conflict between three or four primary colors, Kries divided the process of color vision into a peripheral and a central zone.
Kries-Zonentheorie
[53] supported · niche source
Bipolar cells carry photoreceptor information into the inner retina, where amacrine cells add further temporal and spatial processing.
"Bipolar cells transmit photoreceptor-derived information into the inner retina, where amacrine cells introduce additional temporal and spatial processing"
Guppy color vision: opsin diversity, retinal physiology, plasticity, and evolutionary significance (2026)
[54] supported · reference source
Neurophysiological research since 1966 has confirmed that Hering's three opponent processes actually exist, though his ideas were highly simplified.
"Obwohl Herings Vorstellungen stark vereinfachend waren, konnten diese drei Prozesse tatsächlich nachgewiesen werden. Seit 1966 bestätigen neurophysiologische Untersuchungsergebnisse, dass es vier grundlegende Farbempfindungen gibt."
Gegenfarbtheorie
[55] supported · reference source
In the peripheral zone the photoreceptors pick up three signals, which the central nervous system then recombines into two opposing pairs of primary colors.
"Dabei nimmt die periphere Zone der Sehzellen drei Signale auf. Diese Signale werden in der zentralen Zone, also im Nervensystem, in einem Prozess zu zwei gegensätzlichen Paaren von Grundfarben geformt."
Translation: In this process, the peripheral zone of the visual cells receives three signals. These signals are then formed in the central zone, i.e. in the nervous system, in a process into two opposing pairs of primary colors.
Kries-Zonentheorie
[56] supported · niche source
Ganglion cells are the retina's major output stage, converting local retinal activity into action potentials sent through the optic nerve to higher visual centers.
"Ganglion cells represent a major output stage of the retina, transforming local retinal activity into action potentials that are transmitted through the optic nerve to higher visual centers"
Guppy color vision: opsin diversity, retinal physiology, plasticity, and evolutionary significance (2026)
[57] supported · reference source
The opponent signals yield three dimensions of sensation: brightness, the yellow-blue component, and the red-green component, from which several thousand color types can be distinguished.
"So entstehen, wie auch Hering postulierte, drei Empfindungsdimensionen: 1. Helligkeit, 2. Gelb-Blau-Komponente, 3. Rot-Grün-Komponente, aus denen dann mehrere tausend Farbarten unterschieden werden können."
Gegenfarbtheorie
[58] supported · reference source
Ewald Hering proposed opponent-color pairs (red-green, yellow-blue, black-white), reasoning that no color can be reddish and greenish at once or yellow and blue at once.
"Da keine Farbe zugleich rötlich und grünlich oder gleichzeitig Gelb und Blau ist, nahm er komplementäre Wahrnehmungen an, in denen die Farbwahrnehmung aus einem Rot-Grün-, einem Gelb-Blau- und einem Schwarz-Weiß-Ablauf besteht."
Translation: Since no color is both reddish and greenish, or yellow and blue at the same time, he assumed complementary perceptions, in which color perception consists of a red-green, a yellow-blue and a black-white process.
Kries-Zonentheorie
[59] supported · scholarly source
Rayleigh scattering by atmospheric gases is responsible for the blue colour of the sky under clear conditions.
"the colour of the blue sky under clear conditions"
Relative sky radiance from multi-exposure all-sky camera images (2021)
[60] supported · scholarly source
Air molecules scatter light with a strong wavelength dependence (Rayleigh scattering), which favors blue light and produces the deep blue sky.
"Scattering is given a wavelength (λ) dependence of λ −4 for air molecules (Rayleigh scattering), λ −1 for tropospheric aerosols, and λ +1 for volcanic aerosol particles."
Simulating colors of clear and partly cloudy skies (2005)
[61] supported · reference source
Rayleigh gave an explanation for the blue color of the sky, as part of his work in optics.
"En el campo de la óptica realizó una serie de trabajos sobre la polarización de la luz, contribuyó a la teoría de la radiación del cuerpo negro y logró dar una explicación del color azul del cielo."
Translation: In the field of optics he carried out a series of works on the polarization of light, contributed to the theory of black-body radiation, and managed to give an explanation of the blue color of the sky.
Lord Rayleigh
[62] supported · scholarly source
Tropospheric aerosols, such as smoke particles, scatter with a much weaker wavelength dependence than air molecules, so they scatter blue light less preferentially and add more evenly colored light that dilutes the blue.
"λ −1 for tropospheric aerosols"
Simulating colors of clear and partly cloudy skies (2005)
[63] documented · scholarly source
As haze thickens, the B/R ratio of the sky falls toward 1.0 and the sky shifts from blue to gray.
"にヘイズが濃くなるとB/R比は1.0に接近し,空は青"
Translation: As the haze gets thicker, the B/R ratio approaches 1.0, and the sky changes from blue to gray.
Relations between the Sky Hue and Aerosol Scattering (2009)
[64] supported · primary source
Fine particles matter most for total optical extinction because they scatter light efficiently.
"Fine particles are particularly important in total optical extinction because of their high mass scattering efficiency and absorption cross-sections."
Particle size distributions of wildfire aerosols in the western USA
[65] supported · primary source
Atmospheric aerosols influence the global radiation balance by scattering and absorbing solar radiation.
"Atmospheric aerosols influence the global radiation balance by directly scattering and absorbing solar radiation."
Particle size distributions of wildfire aerosols in the western USA
[66] documented · scholarly source
Fine particles played an important role in controlling visibility in Tianjin, which is the aerosol size range most relevant to scattering light.
"The results show that fine particles played important roles in controlling visibility in Tianjin."
Effect of Aerosols on Visibility and Radiation in Spring 2009 in Tianjin, China (2012)
[67] supported · scholarly source
At constant PM2.5 mass concentration, a larger geometric mean particle diameter gives greater visibility.
"When the mass concentration of PM2.5 is constant, the larger the geometric mean of the particle diameter is, the larger the visibility is."
Study on the relationship between PM2.5 concentration and visibility in Beijing based on light scattering theory (2018)
[68] supported · scholarly source
Higher PM2.5 concentration makes multiple scattering of light more pronounced.
"The result shows that the higher PM2.5 concentration is,the more obvious the multiple scattering effect is."
Study on the relationship between PM2.5 concentration and visibility in Beijing based on light scattering theory (2018)
[69] documented · scholarly source
During haze, the aerosol scattering coefficient rose to about 0.665 per km, versus about 0.213 per km on non-haze days, showing that scattering makes up most of the light extinction.
"The average extinction coefficient and scattering coefficient of atmospheric aerosols were 0.253 1/km and 0.213 1/km in non-haze days, while 0.767 1/km and 0.665 1/km in haze days."
Effect of Aerosols on Visibility and Radiation in Spring 2009 in Tianjin, China (2012)
[70] supported · reference source
Mie scattering is the elastic scattering of electromagnetic waves by spherical objects whose diameter is roughly the wavelength of the radiation, and Lorenz-Mie theory describes it physically.
"Als Mie-Streuung oder auch Lorenz-Mie-Streuung (nach den Physikern Gustav Mie und Ludvig Lorenz ) bezeichnet man die elastische Streuung elektromagnetischer Wellen an sphärischen Objekten, deren Durchmesser in etwa der Wellenlänge der Strahlung entspricht."
Translation: Mie scattering or Lorenz-Mie scattering (named after the physicists Gustav Mie and Ludvig Lorenz) refers to the elastic scattering of electromagnetic waves by spherical objects whose diameter roughly corresponds to the wavelength of the radiation.
Mie-Streuung
[71] supported · reference source
The Tyndall effect makes a medium look whitish and turbid when the scattering particles are larger than the wavelength of light.
"das Medium weißlich trüb erscheinen lassen, wenn sie größer sind."
Translation: let the medium appear whitish and turbid when they are larger.
Tyndall-Effekt
[72] supported · niche source
Near the horizon, light travels through more air and particle-filled layers, so extra Mie scattering from dust and pollution adds white light and makes the blue look paler.
"Near the horizon, light travels through more air and more particle‑filled layers, so additional Mie scattering from dust and pollution adds white light and makes the blue look paler and less saturated."
How Rayleigh Scattering Turns a Blue Sky Into Red/Orange Sunsets Over a Long Atmosphere Path
[73] supported · reference source
The Tyndall effect itself is not responsible for the blue color of the sky.
"Der Effekt ist allerdings selbst nicht für die blaue Farbe des Himmels verantwortlich."
Translation: However, the effect itself is not responsible for the blue color of the sky.
Tyndall-Effekt
[74] supported · niche source
Above the observer there is about 8 miles of atmosphere, while the light reaching the eye from the horizon has travelled through 100 miles or more.
"Above your head is roughly 8 miles of atmosphere, but when looking at the horizon, the light must travel through 100 miles or more of the atmosphere before reaching your eye."
Sky Horizon Science: Why Is The Sky Lighter At The Horizon?
[75] supported · niche source
Looking toward the horizon means viewing through a longer path of air with more particles, and these larger particles add a whitish component that dilutes the intense blue sky.
"Looking toward the horizon means viewing through a longer path of air and more particle‑filled layers that contain dust, pollution, and droplets. These larger particles enhance Mie scattering, adding a whitish component that dilutes the intense blue sky."
How Rayleigh Scattering Turns a Blue Sky Into Red/Orange Sunsets Over a Long Atmosphere Path
[76] supported · reference source
John William Strutt, 3rd Baron Rayleigh, proposed in 1899 that pure air alone, without colloidal particles, causes the scattering that makes the sky blue, the Rayleigh scattering named after him.
"John William Strutt, 3. Baron Rayleigh , postulierte 1899 als erster, dass keine kolloiden Teilchen für das Blau des Himmels benötigt werden, dass vielmehr auch reine Luft die entsprechende Streuung, die nach ihm genannte Rayleigh-Streuung , verursacht."
Translation: John William Strutt, 3rd Baron Rayleigh, postulated in 1899 as the first that no colloidal particles are needed for the blue of the sky, but that rather pure air also causes the corresponding scattering, the Rayleigh scattering named after him.
Tyndall-Effekt
[77] supported · niche source
Mie scattering comes from particles similar in size to light's wavelength, such as water droplets, dust and pollution, and it scatters all visible wavelengths more evenly, producing a whiter, washed-out appearance.
"Mie scattering, by contrast, happens when the particles are similar in size to the wavelength of light, such as water droplets or particles from dust and pollution. These larger particles scatter all visible wavelengths more evenly, creating a whiter, more washed‑out appearance."
How Rayleigh Scattering Turns a Blue Sky Into Red/Orange Sunsets Over a Long Atmosphere Path
[78] supported · niche source
Near the horizon, Mie scattering and repeated Rayleigh scattering wash the blue out toward white, because the sightline runs through more air and the dusty, humid layers near the ground.
"Looking out at the horizon, that same sightline runs through many times more air and through the dustier, more humid layers near the ground, so Mie scattering and repeated Rayleigh scattering wash the blue out toward white."
Sky Horizon Science: Why Is The Sky Lighter At The Horizon?
[79] documented · scholarly source
For fine-mode aerosols, the sky polarization pattern is not sensitive to whether the aerosol absorbs light, so absorption is hard to detect from this pattern alone.
"For fine-mode aerosol, on the other hand, the change of pattern is not sensitive to the absorbing property of aerosol."
Sensitive Research of Scattering and Absorbing Aerosols on Sky Polarization Pattern (2020)
[80] supported · scholarly source
For coarse-mode aerosols, the decrease in downward degree of linear polarization as aerosols turn from scattering to absorbing slows down as aerosol optical depth increases.
"When coarse-mode aerosol changes from scattering to absorbing, the decreasing trend in the sky downward degree-of-linear-polarization largely slows down when aerosol optical depth increases."
Sensitive Research of Scattering and Absorbing Aerosols on Sky Polarization Pattern (2020)