Cassegrain reflector oor Spaans

Cassegrain reflector

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telescopio de Cassegrain

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A third form of reflecting telescope, the "Cassegrain reflector" was devised in 1672 by Laurent Cassegrain.
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Following his death a 24" Cassegrain reflector telescope added to the McMath-Hulbert Observatory was named the F. C. McMath Memorial Telescope.
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The KAO's telescope was a conventional Cassegrain reflector with a 36-inch (91.5 cm) aperture, designed primarily for observations in the 1 to 500 μm spectral range.
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The 1.52 m (60 in) Steward Observatory Telescope is a Cassegrain reflector used for the Mount Lemmon Survey (MLS), which is part of the Catalina Sky Survey (CSS).
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The Cassegrain reflector is named after a published reflecting telescope design that appeared in the April 25, 1672 Journal des sçavans which has been attributed to Laurent Cassegrain.
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These may be integral part of the optical design (Newtonian telescope, Cassegrain reflector or similar types), or may simply be used to place the eyepiece or detector at a more convenient position.
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As with the other Cassegrain-configuration reflectors, the RCT has a very short optical tube assembly and compact design for a given focal length.
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the optics on the Newtonian reflector don't even approach a Schmidt-Cassegrain.
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The West Dome has a 24-inch f/11 Cassegrain reflector purchased by AAI.
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Pictured here is the facility's 0.6-metre Cassegrain reflector telescope, which was installed in 1996.
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Design of dichroic cassegrain reflector at C&X or Ku&X frequency bands
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70m Cassegrain reflector on Alt/Az mount. ~3850 m2 aperture.
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The satellite dish has a secondary Cassegrain reflector.
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A Cassegrain reflector is analyzed at C, X and K bands. Selective behavior is achieved by replacing the reflectors by FSS crosses.
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The key piece of scientific equipment consisted of a Cassegrain reflector telescope with a primary mirror of 12 inches in diameter and a effective focal length of approximately 120 inches.
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Holcomb Observatory and Planetarium The Holcomb Observatory (Indianapolis) has a Physics and Anatomy Department that supports students from Butler University and Indianapolis. The public observatory houses a 38-inch Cassegrain reflector.
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It houses five Schmidt-Cassegrain telescopes, an 18-inch Newtonian reflector, and a 14-inch Schmidt-Cassegrain telescope for research.
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Bushnell offers several kinds of telescopes, producing models of reflector, refractor, and Maksutov-Cassegrain telescopes.
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Laurent Cassegrain in 1672 described the design of a reflector with a small convex secondary mirror to reflect light through a central hole in the main mirror.
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Their Schmidt-Cassegrain telescopes with ACF (Advanced Coma Free) technology are among the best reflector telescopes on the market.
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The most common antenna is the Cassegrain one, which uses as secondary reflector (or subreflector), a hyperboloid, one of its two focuses coincide with the main reflector to ensure that the concentration of energy is directed towards the second focus of the hyperboloid, located much closer to the main structure.
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LLAMA is a Cassegrain ALMA-type telescope, manufactured by Vertex AntennenTechnik GmbH, whose main reflector has a diameter of 12m, a target surface rms accuracy of 15 μm, and a target antenna pointing accuracy of 2 arcsec.
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In order to choose your equipment, you have to consider that there are telescopes for Stars/Planetary (refractors), others for Deep Sky object (reflectors) and others that could give us versatility for both (Smith Cassegrain).
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The INAOE has a modern reflector telescope with a Ritchey-Chrétien optical system, derived from the Cassegrain, built by two mirrors, the primary one with a 2.12 meter diameter and the second is a 50 cm hyperbolic mirror.
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For his design, we have performed a model of a Cassegrain antenna with horn feed in FEKO, and we have simulated the radiation patterns corresponding to the different angles of rotation of the two reflectors around the axis on which they are located.
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25 sinne gevind in 10 ms. Hulle kom uit baie bronne en word nie nagegaan nie.