MAGIC (telescope) - definition. What is MAGIC (telescope)
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%ما هو (من)٪ 1 - تعريف

TWO-TELESCOPE SYSTEM IN THE CANARY ISLANDS
MAGIC (Telescope); Major Atmospheric Gamma-ray Imaging Cherenkov; Major Atmospheric Gamma Imaging Cherenkov Telescopes; Major Atmospheric Gamma Ray Imaging Cherenkov
  • MAGIC on a sunny day
  • active]] control could be seen. However, they are no longer needed for operation.
  • Individual segments of a MAGIC telescope

MAGIC (telescope)         
MAGIC (Major Atmospheric Gamma Imaging Cherenkov Telescopes, later renamed to MAGIC Florian Goebel Telescopes) is a system of two Imaging Atmospheric Cherenkov telescopes situated at the Roque de los Muchachos Observatory on La Palma, one of the Canary Islands, at about 2200 m above sea level. MAGIC detects particle showers released by gamma rays, using the Cherenkov radiation, i.
Refractor         
  • The Apochromatic lens usually comprises three elements that bring light of three different frequencies to a common focus
  • The Yerkes Great refractor mounted at the 1893 World's Fair in Chicago; the tallest, longest, and biggest aperture refractor up to that time.
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  • This 12 inch refractor is mounted in a dome on a mount that matches the Earth's rotation
  • Astronaut trains with camera with large lens
  • Vienna University Observatory]]
  • Touristic telescope pointed to Matterhorn in Switzerland
  • The Greenwich 28-inch refractor is a popular tourist attraction in 21st century London
  • Alvan Clark polishes the big Yerkes achromatic objective lens, over 1 meter across, in 1896.
  • in}} refractor, at [[Yerkes Observatory]], the largest achromatic refractor ever put into astronomical use (photo taken on 6 May 1921, as Einstein was visiting)
TYPE OF OPTICAL TELESCOPE
Refractor; Refractor telescope; Refractive telescope; Galilean Telescope; Refracting Telescope; Galilean telescope; Keplerian telescope; Keplerian Telescope; Refractor Telescope; Kepler refractor; Galileo Telescope; Galileo's telescope; Refractory telescope
·noun Anything that refracts.
II. Refractor ·noun A refracting telescope, in which the image to be viewed is formed by the refraction of light in passing through a convex lens.
Refracting telescope         
  • The Apochromatic lens usually comprises three elements that bring light of three different frequencies to a common focus
  • The Yerkes Great refractor mounted at the 1893 World's Fair in Chicago; the tallest, longest, and biggest aperture refractor up to that time.
  • publisher=Auctor}}</ref>
  • This 12 inch refractor is mounted in a dome on a mount that matches the Earth's rotation
  • Astronaut trains with camera with large lens
  • Vienna University Observatory]]
  • Touristic telescope pointed to Matterhorn in Switzerland
  • The Greenwich 28-inch refractor is a popular tourist attraction in 21st century London
  • Alvan Clark polishes the big Yerkes achromatic objective lens, over 1 meter across, in 1896.
  • in}} refractor, at [[Yerkes Observatory]], the largest achromatic refractor ever put into astronomical use (photo taken on 6 May 1921, as Einstein was visiting)
TYPE OF OPTICAL TELESCOPE
Refractor; Refractor telescope; Refractive telescope; Galilean Telescope; Refracting Telescope; Galilean telescope; Keplerian telescope; Keplerian Telescope; Refractor Telescope; Kepler refractor; Galileo Telescope; Galileo's telescope; Refractory telescope
A refracting telescope (also called a refractor) is a type of optical telescope that uses a lens as its objective to form an image (also referred to a dioptric telescope). The refracting telescope design was originally used in spyglasses and astronomical telescopes but is also used for long-focus camera lenses.

ويكيبيديا

MAGIC (telescope)

MAGIC (Major Atmospheric Gamma Imaging Cherenkov Telescopes, later renamed to MAGIC Florian Goebel Telescopes) is a system of two Imaging Atmospheric Cherenkov telescopes situated at the Roque de los Muchachos Observatory on La Palma, one of the Canary Islands, at about 2200 m above sea level. MAGIC detects particle showers released by gamma rays, using the Cherenkov radiation, i.e., faint light radiated by the charged particles in the showers. With a diameter of 17 meters for the reflecting surface, it was the largest in the world before the construction of H.E.S.S. II.

The first telescope was built in 2004 and operated for five years in standalone mode. A second MAGIC telescope (MAGIC-II), at a distance of 85 m from the first one, started taking data in July 2009. Together they integrate the MAGIC telescope stereoscopic system.

MAGIC is sensitive to cosmic gamma rays with photon energies between 50 GeV (later lowered to 25 GeV) and 30 TeV due to its large mirror; other ground-based gamma-ray telescopes typically observe gamma energies above 200–300 GeV. Gamma-ray astronomy also utilizes satellite-based detectors, which can detect gamma-rays in the energy range from keV up to several GeV.