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About: Wright camera     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:Whole100003553, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)

Type: yago:WikicatCamerasByTypeyago:WikicatOpticalDevicesyago:Artifact100021939yago:Camera102942699yago:Device103183080yago:Equipment103294048yago:Instrumentality103575240yago:Object100002684yago:OpticalDevice103851341yago:PhotographicEquipment103926148yago:PhysicalEntity100001930yago:Whole100003553 New Facet based on Instances of this Class

In astrophotography, the Wright camera design, presented by Franklin Wright (Berkeley, California) in 1935, just a few years after the introduction of the Schmidt camera, was his "short" alternative to the original arrangement. Wright placed the Schmidt corrector at the focal plane, and had the mirror aspherised to cancel coma resulting from the altered aperture stop position (the aperture stop effectively coinciding with the corrector).