Adaptive Optics in Ground Based Telescopes
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WHAT IS ADAPTIVE OPTICS ?

Adaptive optics refers to optical systems which adapt to compensate for optical effects introduced by the medium between the object and its image. In theory a telescope's resolving power is directly proportional to the diameter of its primary light gathering lens or mirror. But in practice , images from large telescopes are blurred to a resolution no better than would be seen through a 20 cm aperture with no atmospheric blurring. At scientifically important infrared wavelengths, atmospheric turbulence degrades resolution by at least a factor of 10.

Space telescopes avoid problems with the atmosphere, but they are enormously expensive and the limit on aperture size of telescopes is quite restrictive. The Hubble Space telescope, the world's largest telescope in orbit , has an aperture of only 2.4 metres, while terrestrial telescopes can have a diameter four times that size.

In order to avoid atmospheric aberration, one can turn to larger telescopes on the ground, which have been equipped with ADAPTIVE OPTICS system. With this setup, the image quality that can be recovered is close to that the telescope would deliver if it were in space. Images obtained from the adaptive optics system on the 6.5 m diameter telescope, called the MMT telescope illustrate the impact
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Messages In This Thread
RE: Adaptive Optics in Ground Based Telescopes - by computer science crazy - 17-09-2009, 12:46 AM
newerasalegermany.com/ pci - by ftwlQlold - 09-07-2014, 11:30 AM
su7f0x5z49i - by 2j06dso9eu - 29-09-2014, 01:59 AM
RE: Adaptive Optics in Ground Based Telescopes - by 4t61xgt7rp - 30-09-2014, 11:15 PM
RE: Adaptive Optics in Ground Based Telescopes - by 8c45ltb6uy - 05-10-2014, 11:40 AM

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