F13839_ANGELINA-XW-B Optoelectronics

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Optics - Reflectors: F13839_ANGELINA-XW-B application field and working principle

F13839_ANGELINA-XW-B is an optical reflective system designed to produce high-quality images in two or three dimensions with superlong focal length. It is primarily used in extragalactic astronomy and astrophotography. The system consists of two mirror elements (primary and secondary mirror) with a focal length of up to 340 times the aperture of the primary mirror.

When light is released from a distant source, it is captured by the primary mirror and converges to the center of the secondary mirror. The converging beam is then reflected back towards the primary mirror, where it is deflected at a dihedral angle to produce a wide field of view. This enables the observer to obtain a large area of deep space with one exposure.

F13839_ANGELINA-XW-B also makes use of classical optical aberrations to reduce the amount of light loss. The aberrations are generated occasionally, due to the deviation of light from the geometric form and the deviation from the ideal form of the image produced. As a result of these aberrations, the image is both blurred and distorted. Additionally, the system maintains high clarity and even distribution of light.

F13839_ANGELINA-XW-B has a number of applications which make it an important tool for astrophotography. It can be used to capture images from deep space like galaxies, star fields, or supernovae. It can also be used to capture wide-field images, making it possible to capture multiple objects in a single exposure. Additionally, the system can be used to view distant regions of the universe which cannot be easily observed with traditional telescope systems.

The working principle of F13839_ANGELINA-XW-B is based on the light interference and light diffraction principle. Light from the distant source is initially captured by the primary mirror. This light is then reflected off the whole reflecting chamber to the center of secondary mirror. The secondary mirror is then deflected at a certain dihedral angle resulting in a wide field of view. Once the light passes through the primary and secondary mirrors, it is diffracted and spread into a set of concentric circles.

The reflecting chamber is equipped with a set of lenses that focus the diffracted light. This light is then further processed by the lens assembly to produce a high-resolution image in both two and three dimensions. The reflections of the primary andsecondary mirrors work to reduce the amount of light loss which would otherwise occur due to the aberrations of the system. This allows the observer to obtain a sharp image with minimum loss of light.

In conclusion, F13839_ANGELINA-XW-B is an advanced optical reflector system designed to produce high-quality images in two and three dimensions with superlong focal length. It has a number of applications in astrophotography, making it a useful tool for capturing images of distant regions of the universe. The principle of operation for the system is based on light interference and diffraction. Additionally, the use of aberrations enables the system to maintain a high degree of clarity in the images produced.

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