Green flash

A green flash is a brief optical phenomenon sometimes visible at the upper edge of the Sun as it rises or sets. Atmospheric refraction bends different wavelengths by slightly different amounts, while scattering and absorption shape which colours reach an observer. With a clear, unobstructed horizon and suitable atmospheric conditions, the final visible sliver may appear green; mirages can alter or intensify the effect. The appearance is fleeting and is not a flash produced by the Sun itself.

Last updated
24 October 2026
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This article was researched and drafted with AI assistance and checked by an automated review pass. It is not guaranteed to be accurate — verify important facts against the references below.

How the effect forms

Near the horizon, sunlight travels through a long path in Earth's atmosphere. Refraction bends the rays, and because the refractive index of air varies with wavelength, colours are displaced by slightly different amounts. The Sun's image can therefore develop narrow colour fringes at its upper and lower edges. As the disk disappears below the horizon, the green part of the upper edge may remain visible briefly after much of the rest of the disk has vanished. Atmospheric scattering and absorption affect the colours that survive; blue and violet are often strongly diminished, allowing green to stand out. The phenomenon is an atmospheric optical effect, not a burst of green light emitted by the Sun.

When it can be seen

Green flashes are most often sought at sunset, though they can also occur at sunrise. A low, unobstructed horizon gives the observer a view of the Sun's final edge; clear air generally improves the chance of seeing the brief colour. The effect commonly lasts only a moment, so a distant sea horizon is a popular viewing location, but a horizon formed by cloud tops or mountains can also provide a sightline. Atmospheric temperature layers can create mirages and reshape the apparent solar image, sometimes making the flash more distinct or changing its form.

Forms and appearances

Observers describe several forms rather than one uniform flash. An inferior-mirage flash occurs close to the horizon; a mock-mirage flash can appear as a narrow strip at the Sun's edge; a subduct flash is associated with an hourglass-shaped solar image under an atmospheric inversion; and a green ray is a rarer beam-like appearance extending above the horizon. These descriptions refer to different atmospheric image distortions and viewing conditions. The green colour is typical but not inevitable: in very clear air, blue or violet may sometimes be visible instead.

Observation and safety

A green flash can be difficult to predict because it depends on both the sightline and the changing atmosphere near the horizon. It is best observed when the Sun is naturally close to the horizon and its disk is about to disappear, without looking directly at the bright disk while it is still above the horizon. Binoculars, telescopes, cameras with optical viewfinders, and other magnifying optics must never be aimed at the Sun without appropriate certified solar filters, since concentrated sunlight can cause serious eye injury.

Key facts

Cause
Wavelength-dependent atmospheric refraction separates the apparent positions of colours near the solar limb; atmospheric scattering and absorption also influence the visible colour.
Timing
The phenomenon may occur at sunrise or sunset and is commonly visible only for a brief moment.
Conditions
A clear view of the horizon and suitable atmospheric conditions increase the chance of seeing it; mirages can modify its appearance.
Forms
Commonly described forms include inferior-mirage, mock-mirage, subduct, and green-ray flashes.
Nature
It is an optical effect of the atmosphere, not a green emission from the Sun.

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References

  1. 1.
    Explaining Green Flashes

    Andrew T. Young, San Diego State University · other · reliability: unverified · retrieved 24 October 2026

    Supports: Explains atmospheric dispersion, extinction, and why green or other short-wavelength colours may appear at sunset.

  2. 2.
    Green Flash

    SKYbrary Aviation Safety · other · reliability: unverified · retrieved 24 October 2026

    Supports: Describes the phenomenon, viewing conditions, mirage-related forms, and typical brief duration.

  3. 3.
    Catching the elusive 'green flash'

    American Association for the Advancement of Science (AAAS) · other · reliability: unverified · retrieved 24 October 2026

    Supports: Summarizes the role of mirages and dispersion and describes several recognized forms.

  4. 4.
    The Green Flash at Sunset

    Nature · other · reliability: unverified · retrieved 24 October 2026

    Supports: Historical scientific discussion identifies refraction, dispersion, and differential scattering as contributors to the phenomenon.

References are suggested by the research engine and may be incomplete. Unverified URLs are omitted rather than guessed.

Article history

  1. Version 124 October 2026 · EditorCreated by Zapia