corrector plate

corrector plate

[kə′rek·tər ‚plāt]
(optics)
A thin lens or system of lenses used to correct the spherical aberration of a spherical lens or the coma of a parabolic lens; used particularly in telescopes such as the Schmidt telescope. Also known as correcting plate.
References in periodicals archive ?
Behind that he mounted a smaller circular plain glass plate of the same substrate to serve as a corrector plate to remove the astigmatism in the guider image introduced by its light passing through the 45[degrees] mirror.
In common with SCTs, Schmidt cameras brought light to a focus using a catadioptric combination of a refracting corrector plate followed by a spherical short-focal-length primary mirror.
The corrector plate bent the light waves in such a way as to eliminate distortion, so that even wide fields could be enlarged steadily.
2 spherical primary mirror, the design incorporates a Schmidt corrector plate that eliminates image-blurring spherical aberration.
The project soon ran into technical difficulties, partly because the astronomers wanted to build two telescopes in one--a Schmidt camera for wide-angle photography, which could be converted into a conventional Cassegrain reflector for spectroscopy when the giant corrector plate was removed.
This is true whether we're talking about a reflector's mirror, a refractor's objective, or the corrector plate of a Maksutov or Schmidt-Cassegrain telescope.
The optical design consists of a full-aperture corrector plate combined with a Mangin primary mirror and 2-element corrector lens, yielding a 60-mm fully illuminated photographic field.
Because the HyperStar lens and your camera are mounted directly on the SCT's corrector plate, they form part of the telescope's "central obstruction.
The XLT in the name refers to the Celestron's StarBright coatings, which are applied to the SCT's front corrector plate and both mirrors, and are designed to maximize the light throughput of the scope.
Compared to Maks, the relatively thin Schmidt corrector plate makes the C6 about 3 pounds lighter, and it requires less time to reach thermal equilibrium when carried from a warm house into the cool night.
A fire extinguisher was found resting on the Schmidt corrector plate, many sharp nails were shoved inside the telescope from the eyepiece side, and the finderscopes were left in various states of disrepair.
The design of the three drive shafts running from motors near the primary mirror to the focus/collimation mechanisms near the corrector plate allows them to freely expand and contract without affecting the separation of the mirrors.