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41 results about "Mangin mirror" patented technology

In optics, a Mangin mirror is a negative meniscus lens with the reflective surface on the rear side of the glass forming a curved mirror that reflects light without spherical aberration. This reflector was invented in 1876 by a French officer Alphonse Mangin as an improved catadioptric reflector for search lights and is also used in other optical devices.

An imaging system with 15° field of view telecentric three mirrors coaxial

InactiveCN102279047AIncreased frame widthImprove Earth Observation CapabilitiesRadiation pyrometryMirrorsMangin mirrorMirror plane
The invention provides a telecentric imaging system with field of view of 15 degrees and three coaxial reflectors, belongs to the space optics technical field, and relates to a telecentric off-axis three-reflector imaging system. A technical problem to be solved is providing a telecentric imaging system with field of view of 15 degrees and three coaxial reflectors. A technical scheme is as follows: the imaging system comprises a main mirror, a second mirror, a third mirror, an aperture diaphragm and an imaging surface, the main mirror, the second mirror, the third mirror and the aperture diaphragm are coaxial, and the main mirror and the third mirror are coplanar; the second mirror is placed on a reflected light path of the main mirror, the third mirror is placed on a reflected light pathof the second mirror, and the aperture diaphragm is placed on a mirror plane edge of the second mirror; in order to realize telecentric image space, a distance from the aperture diaphragm to the third mirror is half of a summit radius of curvature length of the third mirror; in order to realize wide field of view of 15 degrees, the second mirror is a convex spherical mirror, and the main mirror and the third mirror are concave quarticsurface mirrors; a distance from the second mirror to the third mirror is larger than half of a system image space focal length. According to the system, abundant ground resource information is obtained, and the system has low processing and adjusting difficulty.
Owner:CHANGCHUN INST OF OPTICS FINE MECHANICS & PHYSICS CHINESE ACAD OF SCI

Optical path of multispectral polarization scanning radiometer based on reflecting telescope system

ActiveCN104634742AReduced Variation Factors in Polarization Measurement AccuracySmall residual polarizationMaterial analysis by optical meansLight polarisation measurementReflecting telescopeMangin mirror
The invention discloses an optical path of a multispectral polarization scanning radiometer based on a reflecting telescope system. The optical path comprises a pre-posed scanning mirror set, a telescope system and a main measuring optical path, wherein the pre-posed scanning mirror set is composed of a first planar mirror and a second planar mirror both which are orthogonal and installed on a remote sensing platform; the film layers of the first and second planar mirrors are silver reflection films respectively; the telescope system comprises a main mirror, a secondary mirror and a field diaphragm; the main mirror and the second mirror are concave parabolic mirrors and each plated with the a silver reflection film; the main measuring optical path comprises a polarizing component, multiple color separation filters, multiple reflector plates, multiple focusing lenses, multiple narrow band filters and multiple detectors. Because the reflecting telescope system is applied, the difference factors affecting the polarization measurement precision are reduced; the system is low in residual system polarization, wide in spectral range, flexible in amounts and positions of spectrums, high in transmittance, low in processing and installing precision and system cost.
Owner:HEFEI INSTITUTES OF PHYSICAL SCIENCE - CHINESE ACAD OF SCI

Compact type coaxial refraction and reflection type telescope objective

The invention discloses a compact type coaxial refraction and reflection type telescope objective. The surfaces of all components of the telescope objective are spherical surfaces. The telescope objective comprises a front-group concave lens, a front-group positive lens, a main reflecting mirror, a Mangin mirror, a rear-group concave lens and three rear-group positive lenses, wherein the telescopeobjective is in rotational symmetry relative to a main optical axis, and an aperture diaphragm is positioned on a main reflecting mirror; the middle of the front-group concave lens, the middle of thefront-group positive lens and the middle of the main reflecting mirror are independently provided with a hole; after an incident ray from ground scenery is refracted through the front-group lenses, the incident ray reaches the main reflecting mirror; after the incident ray is focused, the incident ray passes through the front surface, the rear surface and the front surface of the Mangin mirror insequence without hindering in sequence; and after the incident ray is refracted by the rear-group concave lens and three rear-group positive lenses in sequence, the incident ray passes through the center hole of the main reflecting mirror without hindering to finally reach an image surface. The telescope objective has the advantages of long focal length, low cost, small volume, light weight, compact structure, good imaging quality, easiness in processing and adjustment and the like.
Owner:SUZHOU UNIV
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