Приклади вживання Primary mirror Англійська мовою та їх переклад на Українською
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To tune in the primary mirror of the title with www.
The MMTO is the home of the MMT(formerly Multiple Mirror Telescope), which currently has a primary mirror 6.5 m in diameter.
To tune in the primary mirror of the site name without www.
The centerpiece of the TMT Observatory is to be a Ritchey-Chrétien telescope with a 30-metre(98 ft)diameter primary mirror.
(The primary mirror is typically quite close to being parabolic, however.).
The Gregorian design solved the problem of viewing theimage in a reflector by allowing the observer to stand behind the primary mirror.
Hubble's primary mirror is 2.4 meters(7 feet, 10.5 inches) across.
She took the Keck Cosmic Web Imager, a new instrumentrecently installed behind the giant Keck telescope in Hawaii, a 10-meter primary mirror.
The VST primary mirror is the larger of the two, with a diameter of 265 cm and a thickness of 14 cm.
By controlling the shape and position of each segment,active optics allows the primary mirror to compensate for changes in wind, temperature, or mechanical stress on the telescope.
The first primary mirror was destroyed in 2002 while being transported from Europe to Chile.
Shortly after the Hubble Space Telescope was deployed in 1990, the observatory's primary mirror was discovered to have an aberration that affected the clarity of the telescope's early images.
The second primary mirror was installed in January 2006 and became fully operational in January 2008.
KH-11 satellites are believed to resemble the Hubble Space Telescope in size and shape, as the satellites were shipped in similar containers,and had comparable primary mirror diameters.
In the Gregorian design, the primary mirror creates a real image before the secondary mirror. .
In a telescope the objective is the lens at the front end ofa refracting telescope(such as binoculars or telescopic sights) or the image-forming primary mirror of a reflecting or catadioptric telescope.
The top half of the segmented, primary mirror can be seen above the inner ground screen that moves with the telescope.
The water circulating in the hydraulic system, and will serve to remove the unused heat or cooling(as a"refrigerator" in a classic case of a heat engine)by evaporation of water from the primary mirror and the storage pools.
The GMT's primary mirror is designed as a composite of seven individual mirrors: six off-axis mirrors and one central-axis mirror. .
A Ritchey- Chrétien telescope(RCT or simply RC)is a specialized variant of the Cassegrain telescope that has a hyperbolic primary mirror and a hyperbolic secondary mirror designed to eliminate off-axis optical errors(coma).
But where Spitzer's primary mirror is only 85 centimetres in diameter, Webb's primary mirror is 6.5 metres, or about 7.5 times larger.
Since then, advances in optical measurement[8] and fabrication[9] have allowed the RCT design to take over- the Hale telescope, dedicated in 1948, turned out to be thelast world-leading telescope to have a parabolic primary mirror.[10].
For instance, the primary mirror is constructed from 91 hexagonal segments, which is less expensive than manufacturing a single large primary. .
Shortly after Hubble was deployed in 1990, the observatory's primary mirror was discovered to have a flaw that affected the clarity of the telescope's early images.
Each primary mirror is composed of 36 hexagonal segments that work together as one single piece of glass-- a revolutionary engineering feat that allows for massive mirrors.
The VST is an alt-azimuthal wide-field survey telescope with a primary mirror diameter of 2.65 meters that was constructed from 2007- 2011 at the ESO Cerro Paranal Observatory, in Chile.
Each primary mirror consists of 36 hexagonal segments that work together as a single piece of glass- a revolutionary technique that enables the achievement of a large mirror. .
In 1636 MarinMersenne proposed a telescope consisting of a paraboloidal primary mirror and a paraboloidal secondary mirror bouncing the image through a hole in the primary, solving the problem of viewing the image.
For example, if the primary mirror will perform a decorative function with color highlights, the mirror for shaving and applying makeup is the way.
An aberration in the primary mirror of the HRI[11] allowed the HRI to spread the light from observations over more pixels without saturating the CCD, effectively obtaining better data.