C11421_IRINA-RS Allicdata Electronics
Allicdata Part #:

C11421_IRINA-RS-ND

Manufacturer Part#:

C11421_IRINA-RS

Price: $ 0.00
Product Category:

Optoelectronics

Manufacturer: Ledil
Short Description: LENS 1POS 24.7MM ROUND OD 11.7MM
More Detail: Lens with Integrated Mount Clear 6°, 12° Spot Cree...
DataSheet: C11421_IRINA-RS datasheetC11421_IRINA-RS Datasheet/PDF
Quantity: 1000
Lead Free Status / RoHS Status: Lead free / RoHS Compliant
Moisture Sensitivity Level (MSL): 1 (Unlimited)
1 +: 0.00000
Stock 1000Can Ship Immediately
$ 0
Specifications
Series: IRINA
Part Status: Obsolete
Lead Free Status / RoHS Status: --
Type: Lens with Integrated Mount
Moisture Sensitivity Level (MSL): --
Color: Clear
Number of LEDs: 1
Lens Style: Round with Flat Top
Lens Size: 24.7mm Dia
Lens Transparency: Clear
Optical Pattern: Spot
Viewing Angle: 6°, 12°
For Use With/Related Manufacturer: Cree
Material: Acrylic
Mounting Type: Adhesive
Description

Due to market price fluctuations, if you need to purchase or consult the price. You can contact us or emial to us:   sales@allicdata.com

Optics have always been a very interesting area of engineering and so too are lenses. This article will provide an overview of the C11421_IRINA-RS application field and working principle.

The C11421_IRINA-RS is a member of a new family of adaptive optics. This new family is based on the Adaptive Optical Array (AOA) technology developed by NASA\'s Jet Propulsion Laboratory. It is used to correct the wavefront of incoming light, in order to provide a more precise image of the object being observed. It is a highly sensitive system that can accurately detect small changes in the wavefront of any observed object and then adjust the optics in order to create a crystal clear image.

The device consists of an array of very small elements called “pixels” which are basically optical detectors. These pixels are connected to a central controller, which in turn is connected to the optics. As the incoming light is received by the array, the pixels measure the wavefront of the light and calculate the specific adjustments which need to be made in order to create a sharper image. The information which is measured by the pixels is then sent to the central controller, which uses the data to adjust the optics accordingly.

The device is capable of detecting and correcting distortions in the wavefront of any object that passes through the optical system. This makes it an ideal tool for many different application fields, such as in telescopes and lenses used in photography. It is used to correct the optical aberrations which can cause the images to be blurred or distorted. By using the C11421_IRINA-RS system, it is possible to produce images with extremely high levels of detail and clarity.

The device is capable of producing images with far greater resolution and detail than traditional lenses. This is because it is able to make very precise corrections to the wavefront of the light, which results in the light being focused more accurately onto the desired target. This means that photographs or images taken with the C11421_IRINA-RS system are much sharper and more detailed than those taken with traditional optics.

The C11421_IRINA-RS system is highly reliable and robust. It has a very low noise floor and is unaffected by environmental factors such as humidity or temperature. It has a very low power consumption, which makes it ideal for use in applications which require very low power but still require a high level of accuracy. This makes it an excellent choice for applications which require the utmost precision and accuracy.

The C11421_IRINA-RS system is easy to install and maintain. All that is required is for it to be connected to the central controller and to the optics, and the system takes care of the rest. This makes it an ideal choice for applications with limited physical space or where power and maintenance are at a premium.

Overall, the C11421_IRINA-RS is an excellent choice for any application where optical precision and accuracy are paramount. The adaptive optics of the system allow for extremely precise imaging, with a low noise floor and highly reliable performance. This makes it ideal for fields such as photography and astronomy.

The specific data is subject to PDF, and the above content is for reference

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