To measure how the Earth’s atmosphere is changing astronomers monitor fluctuations in brightness of a known bright star, but many times no bright star exists in the direction where atmospheric information is needed. To solve this problem, an artificial guide star is created. A beam of laser is projected up through the atmosphere. At about 100 km, the laser beam hits a layer of sodium atoms created by micrometeorites, which vaporize as they enter the upper atmosphere, and excites the sodium atoms. The excited atoms emit a yellow light in all directions, creating a glowing guide star in the upper atmosphere which the astronomer uses to carry measurements.
The blurring effect of the atmosphere is then compensated by employing a special kind of rapidly flexing mirror, a technique known as adaptive optics.
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