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An integrating sphere and a large field of view negative angle uniform light source system based on the integrating sphere

A uniform light source and integrating sphere technology, applied in spectrometry/spectrophotometry/monochromator, photometry, optical radiation measurement, etc., can solve the problems of ultra-wide-angle camera radiation calibration difficulties and achieve precise adjustment Effect

Inactive Publication Date: 2017-07-28
XI'AN INST OF OPTICS & FINE MECHANICS - CHINESE ACAD OF SCI
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Problems solved by technology

[0011] In order to solve the problem of difficult radiometric calibration of ultra-wide-angle cameras (≥150°), combined with the principle of radiometric calibration of conventional cameras, the present invention proposes an integrating sphere for a uniform light device, and a large field of view negative-angle uniform light source based on the integrating sphere A system that can effectively perform radiometric calibration of ultra-wide-angle cameras in the laboratory

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  • An integrating sphere and a large field of view negative angle uniform light source system based on the integrating sphere
  • An integrating sphere and a large field of view negative angle uniform light source system based on the integrating sphere
  • An integrating sphere and a large field of view negative angle uniform light source system based on the integrating sphere

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Embodiment Construction

[0038] The present invention will be described in detail below in conjunction with the accompanying drawings.

[0039] figure 1 Shown is the structure and working principle diagram of the integrating sphere provided by the present invention. The integrating sphere includes a hollow sphere and a light entrance hole and a light exit hole arranged on the hollow sphere. The hollow sphere includes a front hemisphere and a rear hemisphere. In the body, there are one or more light holes located on the wall of the front hemisphere, and the light entering from the light holes can be directly projected onto the wall of the light hole.

[0040] figure 2 Shown is a large field of view negative angle uniform light source system based on the integrating sphere of the present invention. In addition to the integrating sphere, the system also includes a light source system and a spectrum detector. The light source system includes a plurality of light source lamp assemblies, a plurality of ...

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Abstract

The present invention provides an integrating sphere and a large field of view negative angle uniform light source system based on the integrating sphere. For the sphere and the rear hemisphere, the light exit hole is sunken toward the back hemisphere, and the sunken light exit hole is still located in the front hemisphere. The number of light entrance holes is one or more and they are located on the wall of the front hemisphere. Light can be directly projected onto the hole wall of the light exit hole. The large-field-of-view negative-angle uniform light source system of the present invention utilizes the principle of an integrating sphere, combined with remote sensing camera radiation calibration technology, and for the first time breaks through the design of a super-large field-of-view negative-angle uniform illumination system, and its outgoing light simulation angle can be extended to 220°.

Description

technical field [0001] The invention relates to a uniform light source system with a large field of view, which can be used for radiation calibration of a camera with a large field of view, and can also be used for uniformity calibration of a CCD detector. Background technique [0002] Spacecraft and remote sensors need to be radiated before launch. The purpose is to calibrate the radiance received by the instrument under typical working conditions, provide working parameters for setting the camera, and establish the relationship between the input radiance at the entrance pupil of the camera and the digital output. quantitative relationship. In order to obtain images with appropriate exposure for ground targets with different radiances (changing with the sun's zenith angle and the average reflectance of ground objects), the exposure time of the detector and the gain of its amplifier must be selected reasonably. In order to obtain the best final image possible, careful radio...

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Application Information

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Patent Type & Authority Patents(China)
IPC IPC(8): G01J1/00G01J1/04G01J3/02G01J3/28
Inventor 徐亮赵建科刘峰周艳杨菲郭毅许丹张翰文何郧
Owner XI'AN INST OF OPTICS & FINE MECHANICS - CHINESE ACAD OF SCI