Skyglow

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This photo of New York City shows excessive Sky glow.
This photo of New York City shows excessive Sky glow.
Ciudad de México at night, with a brightly illuminated sky.
Ciudad de México at night, with a brightly illuminated sky.
Los Angeles at night, with a brightly illuminated sky.
Los Angeles at night, with a brightly illuminated sky.

Skyglow (or sky glow), is a kind of light pollution, visible by the "glowing" effect seen in the skies over many cities and towns.

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[edit] Negative effects

Skyglow is a prime problem for astronomers, because it reduces contrast in the night sky to the extent where it may become impossible to see even the brightest stars. (However, most professional observatories have technical means for removing certain wavelengths of light from their images. Specifically, the wavelength of low-pressure sodium lamps is well-known and easy for processing software to pick out.) Ordinary people also miss out. Due to skyglow, many people who live in urban areas cannot see the Milky Way, our own galaxy. Fainter sights like the Zodiacal Lights and the Andromeda Galaxy are nearly impossible to resolve even with telescopes.

[edit] Causes

There are several causes of sky glow. These causes mainly differ in source. For example, public lighting provides a different form of light pollution than do attention-grabbing strobe lamps, and these differ from commerical lighting installations. Light from electric lamps shines onto reflective surfaces like the ground or streets and then bounce into the sky. The light is then refracted in the surrounding atmosphere. This refraction is what makes sky glow.

[edit] Mechanism

This refraction is strongly related to the wavelength of the light. Rayleigh scattering, which makes the sky appear blue in the daytime, also affects light that comes from the earth into the sky and is then redirected to become sky-glow, seen from the ground. As a result, blue light contributes significantly more to sky-glow than an equal amount of yellow light. A simple metric for this phenomenon is the Rayleigh Scatter Index, discussed in[1] a brief article and [2] a 2003 presentation to both the IDA Conference and the IESNA, which indicates that high pressure sodium sources produce roughly one-third to one-half of the skyglow that typical metal halide sources do, based on the same amount of light entering the atmosphere.

[edit] Measuring sky glow

Astronomers have used the Bortle Dark-Sky Scale to measure sky glow ever since it was published in Sky & Telescope magazine.[1] The Bortle Scale rates the darkness of the sky, inhibited by sky glow, on a scale of one to nine, providing a detailed description of each position on the scale.

[edit] External links

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