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Wavefront Sensors

SID4 UHR Ultra-High-Resolution wavefront sensor is adapted for optics metrology needs. It combines the SID4 ease of implementation with high sampling and resolution. Its large aperture allows to get a live wavefront measurement over the complete sample under test. The SID4 UHR is optimized for surface inspection (roughness, high ...

Specifications

Wavelength Range: 400-1100nm
# Pixels (Width): 554
# Pixels (Height): 554
Lenslet Pitch: 27.6 um
Wavefront Accuracy: Other
Designed for life science and material inspection microscopes, SID4-sC8 brings fast, accurate and truly quantitative phase measurement in a compact, plug-and-play solution. Biologists will benefit from label-free cell imaging, high sensitivity and automatic segmentation, while material scientists will have access to accurate ...

Specifications

Wavelength Range: 400-1000nm
# Pixels (Width): 852
# Pixels (Height): 720
Lenslet Pitch: 19.5 um
Wavefront Accuracy: <= lambda/20
The SID4 HR brings ultra-high phase sampling (416 x 360) and high dynamic range (500 µm PV) to the most demanding wavefront measurement applications. Its large aperture and extreme wavefront sensitivity makes it perfectly suited to direct measurement of large diverging beams without relay optics.

Specifications

Wavelength Range: 400-1100nm
# Pixels (Width): 360
# Pixels (Height): 416
Lenslet Pitch: 24 um
Wavefront Accuracy: <= lambda/20
The SID4 DWIR is the first off-the-shelf high-resolution wavefront sensor for dual-band infrared from 3 to 5 µm and 8 to 14 µm. It is well suited to characterize IR optics, blackbody sources, 3.39 µm or 10.6 µm laser beams, and systems.

Specifications

Wavelength Range: 3000-14000nm
# Pixels (Width): 160
# Pixels (Height): 120
Lenslet Pitch: 60 um
Wavefront Accuracy: <= lambda/20
The SID4 SWIR HR wavefront sensor integrates Phasics' patented technology with an InGaAs detector. Thanks to its ultra-high spatial resolution (160 x 128 phase pixels) and high sensitivity, it offers accurate wavefront measurement from 900 nm to 1.7 µm. SID4 SWIR HR is an innovative solution for testing SWIR optical systems ...

Specifications

Wavelength Range: 900-1700nm
# Pixels (Width): 160
# Pixels (Height): 128
Lenslet Pitch: 60 um
Wavefront Accuracy: <= lambda/15
ALPAO Shack–Hartmann (SH) wavefront sensors (WFS) are the only range of WFS specifically designed for Adaptive Optics (AO). They feature excellent performances to fit with every adaptive optics system. Sensitivity, speed, and spectral range can be chosen depending on your needs. All ALPAO SHs perfectly fit with ALPAO Deformable ...

Specifications

Wavelength Range: 350-2000nm
# Pixels (Width): --
# Pixels (Height): --
Lenslet Pitch: -- um
Wavefront Accuracy: Other
Dynamic Optics Shack Hartmann wavefront sensor offers the best compromise between fast acquisition (up to 1KHz with 8 x 8 centroids) and ease of use.

Specifications

Wavelength Range: 350-1000nm
# Pixels (Width): 1535
# Pixels (Height): 1216
Lenslet Pitch: 150 um
Wavefront Accuracy: Other
Measuring or even controlling quickly varying optical aberrations with a high spatial resolution is currently connected with high cost for processing hardware and sensor equipment. JOÃO is a Shack-Hartmann wavefront sensor that breaks these limits. Connected to an off-the-shelf Personal Computer, JOÃO keeps track of ...

Specifications

Wavelength Range: 400-950nm
# Pixels (Width): 820
# Pixels (Height): 740
Lenslet Pitch: 300 um
Wavefront Accuracy: <= lambda/10
The HASO LIFT 272 wavefront sensor is as powerful as its counterpart in terms of accuracy and dynamic range, while offering an unequaled resolution of 272 x 200 phase points. This allows the HASO LIFT 272 to provide high-level of performance for applications requiring high accuracy, high dynamic range and high spatial resolution. It ...

Specifications

Wavelength Range: 400-800nm
# Pixels (Width): --
# Pixels (Height): --
Lenslet Pitch: -- um
Wavefront Accuracy: Other
Providing outstanding performance, the HASO Wavefront Sensor family is used in the most demanding applications in optical metrology, free-space communication and laser diagnostics worldwide. The HASO SWIR is a wavefront sensor based on an InGaAs camera, offering high accuracy, large dynamic range and high-speed acquisition frequency. ...

Specifications

Wavelength Range: 900-1700nm
# Pixels (Width): -
# Pixels (Height): -
Lenslet Pitch: - um
Wavefront Accuracy: Other
Providing outstanding performance, the HASO4 FAST wavefront sensor is recommended for optical metrology, that needs high speed and high wavefront measurement accuracy, adaptive optics and free-space communication. We offer a unique combination of expertise in high quality microlens production, software development and accurate ...

Specifications

Wavelength Range: 400-900nm
# Pixels (Width): -
# Pixels (Height): -
Lenslet Pitch: - um
Wavefront Accuracy: Other
Providing outstanding performance, the HASO Wavefront Sensor family is used in the most demanding applications in optical metrology, microscopy and laser diagnostics worldwide. We offer a unique combination of expertise in high quality microlens production, software development and accurate factory calibrations.The HASO4 FIRST ...

Specifications

Wavelength Range: 400-1100nm
# Pixels (Width): -
# Pixels (Height): -
Lenslet Pitch: - um
Wavefront Accuracy: Other
First of all the HASO4 Broadband wavefront sensor is our most versatile . This newly-released second edition features the new SpotTracker technology. It also provides absolute wavefront and tilt information, eliminating alignment requirements. Providing outstanding performance, the HASO Wavefront Sensor family is besides that used in ...

Specifications

Wavelength Range: 350-1100nm
# Pixels (Width): -
# Pixels (Height): -
Lenslet Pitch: - um
Wavefront Accuracy: Other
A great choice for the most demanding SWIR optical metrology applications, the HASO SWIR LIFT 160 wavefront sensor provides the highest resolution in SWIR, and advanced features such SpotTracker for alignment. It also instantly combines with any other compatible instrument and accessory in the Optical Engineer Companion range. The ...

Specifications

Wavelength Range: 1050-1700nm
# Pixels (Width): --
# Pixels (Height): --
Lenslet Pitch: -- um
Wavefront Accuracy: Other
The HASO LIFT 680 wavefront sensor is as powerful as its counterpart in terms of accuracy and dynamic range, while offering an unequaled resolution of 680 x 504 phase points. Providing outstanding performance, the HASO wavefront sensor family is used worldwide in the most demanding applications in optical metrology, industrial ...

Specifications

Wavelength Range: 400-600nm
# Pixels (Width): -
# Pixels (Height): -
Lenslet Pitch: - um
Wavefront Accuracy: Other

Frequently Asked Questions

A Shack-Hartmann wavefront sensor is a device used to measure the wavefront of a light beam. It works by splitting the incoming light into multiple smaller beams, measuring the deviations of these smaller beams, and reconstructing the overall wavefront.

Shack-Hartmann wavefront sensors work by passing incoming light through an array of small lenses, or lenslets. Each lenslet focuses the light into a spot. The position of these spots is then compared to a reference, allowing the sensor to calculate the slope of the wavefront across each lenslet. The full wavefront shape can then be reconstructed.

Shack-Hartmann wavefront sensors have a variety of applications, including adaptive optics (in telescopes and ophthalmology), laser beam characterization, testing and quality control of optical components, and in the study of fluid and thermal dynamics.

The accuracy of a Shack-Hartmann wavefront sensor largely depends on the quality of the lenslet array and the resolution of the detector. Higher resolution detectors and high-quality lenslet arrays can provide more accurate measurements. However, factors such as noise, alignment errors, and environmental factors can also impact the accuracy.

Shack-Hartmann wavefront sensors offer several advantages. They are relatively simple and compact, require few optical components, and can work with a wide range of light sources. In addition, they can measure large wavefront slopes, making them useful in a wide range of applications.

Yes, Shack-Hartmann sensors can be affected by atmospheric conditions, particularly when used in astronomy. Atmospheric turbulence can distort the wavefront of incoming light, affecting the sensor's measurements. Adaptive optics systems, which often use Shack-Hartmann sensors, are designed to correct for these distortions.

Shack-Hartmann sensors are a critical component in many adaptive optics systems. They provide real-time measurements of the wavefront errors caused by atmospheric turbulence or other factors. The adaptive optics system can then adjust a deformable mirror to correct these errors, improving image quality.

When selecting a Shack-Hartmann sensor, you should consider factors such as the required wavefront measurement accuracy, the sensor's dynamic range, the light source wavelength, the desired measurement speed, and the environmental conditions in which the sensor will be used.

Regular cleaning and inspection are important for maintaining a Shack-Hartmann sensor. Dust or other particles can obstruct the lenslets and affect measurements. In addition, it's important to ensure the sensor is properly aligned and calibrated. Specific maintenance procedures can vary based on the specific model of the sensor.

There are 15 different Wavefront Sensors from various suppliers and manufacturers listed in this category. In just a few clicks you can compare different Wavefront Sensors with each other and get an accurate quote based on your needs and specifications.

Understanding Shack-Hartmann Wavefront Sensors: A Brief Technical Overview

Introduction: Shack-Hartmann wavefront sensors play a pivotal role in various fields, from astronomy to adaptive optics. This technical summary delves into the fundamental principles, applications, and advancements of Shack-Hartman wavefront sensors, shedding light on their importance and potential.

Overview of Shack-Hartmann Wavefront Sensors: Shack-Hartmann wavefront sensors are optical devices that measure the shape and quality of light waves by analyzing their wavefront distortion. Comprising an array of micro lenses, these sensors divide the incoming light into small segments, each corresponding to a specific region of the wavefront. By measuring the displacement of these focal spots, the sensor can reconstruct the wavefront, providing valuable insights into optical aberrations and enabling correction techniques.

Principle of Operation: The core principle behind Shack-Hartmann wavefront sensors is based on the concept of wavefront sensing through lenslet arrays. When a wavefront passes through the sensor, it encounters the array of micro lenses, which refract the light onto a detector array. Each lenslet focuses the incoming light onto a unique spot, the position of which indicates the local tilt and phase of the wavefront. By analyzing the displacement of these spots, the wavefront shape and aberrations can be determined.

Applications in Adaptive Optics: Shack-Hartmann wavefront sensors are extensively used in adaptive optics systems, which are employed in astronomy, microscopy, laser beam shaping, and free-space optical communications. In astronomy, these sensors provide real-time measurements of atmospheric turbulence-induced wavefront distortions, enabling the precise adjustment of deformable mirrors to counteract these effects. In microscopy, Shack-Hartmann sensors aid in the correction of sample-induced aberrations, enhancing image quality. Moreover, these sensors find applications in laser beam characterization, ensuring optimal performance and uniformity.

Advancements and Innovations: Over the years, Shack-Hartmann wavefront sensors have undergone significant advancements. Techniques such as dual-plate and multi-wavelength wavefront sensing have been developed to improve accuracy and mitigate certain limitations. Additionally, the integration of liquid crystal devices and adaptive optics into Shack-Hartmann sensors has led to dynamic wavefront correction capabilities. Miniaturization of the sensor has also been achieved, enabling their integration into compact devices and portable systems. These innovations expand the applications of Shack-Hartmann wavefront sensors and enhance their versatility in various domains.

Conclusion: Shack-Hartmann wavefront sensors offer invaluable insights into the wavefront properties of light, enabling precise wavefront measurements, aberration characterization, and real-time correction. Their widespread adoption in adaptive optics systems and other fields underscores their significance. As advancements continue to push the boundaries of performance and miniaturization, Shack-Hartmann sensors are poised to play an increasingly vital role in optimizing optical systems across diverse applications.

Did You know?

Necessity is indeed the mother of invention; a sentiment that perfectly encapsulates the story of the Shack-Hartmann sensor. In the late 1960s, Roland Shack and Ben Platt, based at the Optical Science Center at the University of Arizona, ingeniously modified a Hartmann screen. They replaced its apertures with an array of miniature lenses, or 'lenslets', aiming to enhance the quality of satellite imagery taken from Earth. From that point onward, the Shack-Hartmann sensor has found utility in a diverse range of settings. Its applications stretch from refining astronomical images of the vast cosmos to more terrestrial tasks, such as measuring aberrations in the human eye. This technique has since gained global acceptance, with hundreds of millions of astronomical images improved, and it has contributed to the success of millions of corrective eye surgeries. These surgeries rely on the precise characterization of patient's eyes enabled by the Shack-Hartmann sensor, facilitating the treatment of complex refractive errors. We can expect this trend to continue in the coming years, further enhancing vision and improving lives.