Science, Tech, Math › Science The Green Flash Phenomenon and How to See It Share Flipboard Email Print © Roger Ressmeyer/Corbis/VCG / Getty Images Science Astronomy An Introduction to Astronomy Important Astronomers Solar System Stars, Planets, and Galaxies Space Exploration Chemistry Biology Physics Geology Weather & Climate by Anne Marie Helmenstine, Ph.D. Dr. Helmenstine holds a Ph.D. in biomedical sciences and is a science writer, educator, and consultant. She has taught science courses at the high school, college, and graduate levels. Updated July 02, 2019 The green flash is the name of a rare and interesting optical phenomenon where a green spot or flash is visible at the top edge of the sun at sunrise or sunset. Although less common, the green flash may also be seen with other bright bodies, such as the Moon, Venus, and Jupiter. The flash is visible to the naked eye or photographic equipment. The first color photograph of the green flash was taken at sunset by D.K.J. O'Connell in 1960 from the Vatican Observatory. How the Green Flash Works At sunrise or sunset, light from the sun travels through a thicker column of air before reaching the viewer than when the star is higher in the sky. The green flash is a type of mirage in which the atmosphere refracts sunlight, breaking it into different colors. The air acts as a prism, but not all colors of light are visible because some wavelengths are absorbed by the molecules before the light reaches the viewer. Green Flash Versus Green Ray There is more than one optical phenomenon that can make the Sun appear green. The green ray is a very rare type of green flash that shoots up a beam of green light. The effect is seen at sunset or just afterward when the green flash occurs in a hazy sky. The ray of green light is typically a few degrees of arc high in the sky and can last for several seconds. How to See the Green Flash The key to seeing the green flash is to view sunrise or sunset at a distant, unobstructed horizon. The most common flashes are reported over the ocean, but the green flash can be viewed from any altitude and over land as well as sea. It's regularly seen from the air, particularly in an aircraft traveling west, which delays sunset. It helps if the air is clear and stable, although the green flash has been observed as the sun rises or sets behind mountains or even clouds or a fog layer. Slight magnification, as through a cell phone or camera, generally makes the green rim or flash visible on top of the sun at sunrise and sunset. It's important to never view the unfiltered sun under magnification, as permanent eye damage may result. Digital devices are a safer way to view the sun. If you're viewing the green flash with your eyes rather than a lens, wait until the sun is just rising or has partially set. If the light is too bright, you won't see the colors. The green flash is generally progressive with respect to color/wavelength. In other words, the top of the solar disc appears yellow, then yellow-green, then green, and possibly blue-green. Atmospheric conditions can produce different types of green flashes: Type of Flash Usually Viewed From Appearance Conditions Inferior-mirage Flash sea level or low elevations Oval, flattened disc, Joule's "last glimpse", usually 1-2 seconds duration Occurs when the surface is warmer than the air above it. Mock-mirage Flash more likely viewed the higher it's seen above the inversion, but brightest just above the inversion The upper rim of the sun appears as thin strips. Green strips last 1-2 seconds. Occurs when the surface is cooler than the air above it and the inversion is below the viewer. Sub-duct Flash at any height, but only within a narrow range below the inversion The top part of an hourglass-shaped sun appears green for as long as 15 seconds. Seen when the observer is below an atmospheric inversion layer. Green Ray sea level A green beam of light appears to shoot up from the top center of the sun as it sets or just after it sinks below the horizon. Seen when a bright green flash is present and there is hazy air to produce the column of light. Blue Flash Very rarely, refraction of sunlight through the atmosphere may be sufficient to produce a blue flash. Sometimes the blue flash stacks on top of the green flash. The effect is best seen in photographs rather than with the eye, which is not very sensitive to blue light. The blue flash is so rare because blue light is generally scattered by the atmosphere before it reaches the viewer. The Green Rim When an astronomical object (i.e., the Sun or Moon) sets on the horizon, the atmosphere acts as a prism, separating the light into its component wavelengths or colors. The upper rim of the object may be green, or even blue or violet, while the lower rim is always red. This effect is most often seen when the atmosphere contains a lot of dust, smog, or other particles. However, the particles that make the effect possible also dim and redden the light, making it tricky to see. The colored rim is very thin, so it's difficult to discern with the naked eye. It can be seen better in photographs and videos. The Richard Evelyn Byrd Antarctic expedition reported seeing the green rim and possibly the green flash, lasting for about 35 minutes in 1934. Continue Reading See Why the Sky Is Blue and Sunset Is Red With This Easy Experiment How to Use Your New Telescopes to View Planets The "Impossible Colors" Your Brain Sees but Your Eyes Can't Perceive Why the Sun Looks Yellow When It's Really Not Stargazing Through the Year: A Month-by-Month Astronomy Calendar It's True, Skies Are More Blue in Fall The Visible Spectrum: Wavelengths and Colors Why Magenta Is Not a Color of the Spectrum How Solar Flares Work and the Risks They Pose How Do Astronomers Use Light? 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