FILTER PRODUCTS

to
to
to
to
to
to

FILTER PRODUCTS

to
to
to
to
to
to

Deformable Mirrors

Bertin Alpao Deformable Mirrors (DMs) feature large strokes, high dynamic motion and an excellent optical quality. Bertin Alpao DMs are providing state-of-the-art performances which will meet and exceed your requirements for fast and accurate wavefront corrections.

Specifications

Number Of Actuators: 241
Wavefront Tip-Tilt Stroke (PtV): 10 um
Actuator Pitch: 1500 um
Pupil Size (Clear Aperture): 26.5 mm
Surface Quality (RMS): 7 nm
Bertin Alpao Deformable Mirrors (DMs) feature large strokes, high dynamic motion and an excellent optical quality. Bertin Alpao DMs are providing state-of-the-art performances which will meet and exceed your requirements for fast and accurate wavefront corrections. 

Specifications

Number Of Actuators: 37
Wavefront Tip-Tilt Stroke (PtV): 40 um
Actuator Pitch: 800 um
Pupil Size (Clear Aperture): 5.6 mm
Surface Quality (RMS): 7 nm
mu-DM is a versatile, single-piece design, electromagnetic deformable mirror, which can be implemented in an open-loop or along with a wavefront sensor in a closed-loop setting.  mu-DM is a Deformable Mirror (DM)  containing 91 electromagnetic actuators organized in a centro-symmetrical pattern. The main highlights of this DM ...

Specifications

Number Of Actuators: 91
Wavefront Tip-Tilt Stroke (PtV): 40 um
Actuator Pitch: 10 um
Pupil Size (Clear Aperture): 15 mm
Surface Quality (RMS): 7 nm
ILAO STAR  Deformable Mirror is the most advanced mechanical actuator-based deformable mirror dedicated to ultra-intense lasers. It combines already proven principles from the previous generations of mechanical deformable mirrors with innovative developments fostered by tens of customers.

Specifications

Number Of Actuators: 19
Wavefront Tip-Tilt Stroke (PtV): 3 um
Actuator Pitch: 50 um
Pupil Size (Clear Aperture): 16 mm
Surface Quality (RMS): 10 nm
The Boston Micromachines Hex Class Deformable Mirrors offer an alternative to continuous and discrete segmented devices. Well suited for an array of applications from in vivo microscopy to high resolution astronomy, the Hex mirror architecture has the ability to tip, tilt and piston multiple segments for alternative wavefront control.

Specifications

Number Of Actuators: 1011
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 375 um
Pupil Size (Clear Aperture): 11.6 mm
Surface Quality (RMS): 40 nm
The Kilo-DM deformable mirrors: A high performance wavefront corrector for demanding applications in astronomy, laser communications and imaging through scattering media.The Kilo-DM deformable mirror is an enabling component for precise, high speed, high resolution wavefront control. With 952 actuators controlled to under 1nm of ...

Specifications

Number Of Actuators: 952
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 400 um
Pupil Size (Clear Aperture): 13.2 mm
Surface Quality (RMS): 30 nm
ONE OF OUR UNIQUE FEATURES — WATER COOLED BIMORPH MIRRORS FOR HIGH POWER LASERS, TO ELIMINATE THE RISK OF THERMAL DAMAGE UP TO 50 KW/CM2.

Specifications

Number Of Actuators: 512
Wavefront Tip-Tilt Stroke (PtV): 30 um
Actuator Pitch: 8 um
Pupil Size (Clear Aperture): 20 mm
Surface Quality (RMS): Not Specified
The +K-DM Family of deformable mirrors: High spatial-resolution wavefront correctors for next generation applications in astronomy and laser communications. Boston Micromachines Corporation is leading the industry in high actuator‐count MEMS deformable mirror technology. These mirrors are fielded at prominent astronomical facilities ...

Specifications

Number Of Actuators: 2048
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 400 um
Pupil Size (Clear Aperture): 20 mm
Surface Quality (RMS): 30 nm
The 492-DM deformable mirrors: A high performance wavefront corrector for astronomy and imaging applications. The 492-DM is an enabling component for precise, high speed, high resolution wavefront control. With 492 actuators controlled to under 1 nm of precision and no hysteresis, this system is ideal for demanding applications in ...

Specifications

Number Of Actuators: 492
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 400 um
Pupil Size (Clear Aperture): 9.2 mm
Surface Quality (RMS): 30 nm
The Multi-DM: A versatile, robust deformable mirror system for advanced wavefront control The popular Multi-DM offers sophisticated aberration compensation in an easy-to use package. With 140 precisely controlled elements and low inter-actuator coupling, this system is ideal for a broad range of applications including microscopy, ...

Specifications

Number Of Actuators: 140
Wavefront Tip-Tilt Stroke (PtV): 5.5 um
Actuator Pitch: 300 um
Pupil Size (Clear Aperture): 4.95 mm
Surface Quality (RMS): 30 nm
The Multi-DM deformable mirror: A versatile, robust deformable mirror system for advanced wavefront control The popular Multi-DM offers sophisticated aberration compensation in an easy-to use package. With 140 precisely controlled elements and low inter-actuator coupling, this system is ideal for a broad range of applications ...

Specifications

Number Of Actuators: 140
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 400 um
Pupil Size (Clear Aperture): 4.4 mm
Surface Quality (RMS): 30 nm
The Kilo-DM deformable mirror: A high performance wavefront corrector for demanding applications in astronomy, laser communications and imaging through scattering media.The Kilo-DM deformable mirror is an enabling component for precise, high speed, high resolution wavefront control. With 952 actuators controlled to under 1nm of ...

Specifications

Number Of Actuators: 952
Wavefront Tip-Tilt Stroke (PtV): 1.5 um
Actuator Pitch: 300 um
Pupil Size (Clear Aperture): 9.9 mm
Surface Quality (RMS): 30 nm
The 492-DM deformable mirror: A high performance wavefront corrector for astronomy and imaging applications. The 492-DM is an enabling component for precise, high speed, high resolution wavefront control. With 492 actuators controlled to under 1 nm of precision and no hysteresis, this system is ideal for demanding applications in ...

Specifications

Number Of Actuators: 492
Wavefront Tip-Tilt Stroke (PtV): 1.5 um
Actuator Pitch: 300 um
Pupil Size (Clear Aperture): 6.9 mm
Surface Quality (RMS): 30 nm
The Boston Micromachines Hex Class DeformableMirrors offer an alternative to continuous and discrete segmented devices. Well suited for an array of applications from in vivo microscopy to high resolution astronomy, the Hex mirror architecture has the ability to tip, tilt and piston multiple segments for alternative wavefront control.

Specifications

Number Of Actuators: 507
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 375 um
Pupil Size (Clear Aperture): 8.3 mm
Surface Quality (RMS): 40 nm
The Boston Micromachines Hex Class DeformableMirrors offer an alternative to continuous and discrete segmented devices. Well suited for an array of applications from in vivo microscopy to high resolution astronomy, the Hex mirror architecture has the ability to tip, tilt and piston multiple segments for alternative wavefront control.

Specifications

Number Of Actuators: 111
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 375 um
Pupil Size (Clear Aperture): 3.8 mm
Surface Quality (RMS): 40 nm
The +K-DM Family of deformable mirrors: High spatial-resolution wavefront correctors for next generation applications in astronomy and laser communications. Boston Micromachines Corporation is leading the industry in high actuator‐count MEMS deformable mirror technology. These mirrors are fielded at prominent astronomical facilities ...

Specifications

Number Of Actuators: 4092
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 400 um
Pupil Size (Clear Aperture): 25 mm
Surface Quality (RMS): 30 nm
The +K-DM Family deformable mirrors: High spatial-resolution wavefront correctors for next generation applications in astronomy and laser communications. Boston Micromachines Corporation is leading the industry in high actuator‐count MEMS deformable mirror technology. These mirrors are fielded at prominent astronomical facilities ...

Specifications

Number Of Actuators: 3063
Wavefront Tip-Tilt Stroke (PtV): 1.5 um
Actuator Pitch: 300 um
Pupil Size (Clear Aperture): 18.6 mm
Surface Quality (RMS): 40 nm
The +K-DM Family of deformable mirrors: High spatial-resolution wavefront correctors for next generation applications in astronomy and laser communications. Boston Micromachines Corporation is leading the industry in high actuator‐count MEMS deformable mirror technology. These mirrors are fielded at prominent astronomical facilities ...

Specifications

Number Of Actuators: 3063
Wavefront Tip-Tilt Stroke (PtV): 1.5 um
Actuator Pitch: 300 um
Pupil Size (Clear Aperture): 18.6 mm
Surface Quality (RMS): 30 nm
The +K-DM Family of deformable mirrors: High spatial-resolution wavefront correctors for next generation applications in astronomy and laser communications. Boston Micromachines Corporation is leading the industry in high actuator‐count MEMS deformable mirror technology. These mirrors are fielded at prominent astronomical facilities ...

Specifications

Number Of Actuators: 2048
Wavefront Tip-Tilt Stroke (PtV): 1.5 um
Actuator Pitch: 400 um
Pupil Size (Clear Aperture): 20 mm
Surface Quality (RMS): 30 nm
The Boston Micromachines Hex Class Deformable Mirrors offer an alternative to continuous and discrete segmented devices. Well suited for an array of applications from in vivo microscopy to high-resolution astronomy, the Hex deformable mirror architecture has the ability to tip, tilt and piston multiple segments for alternative ...

Specifications

Number Of Actuators: 111
Wavefront Tip-Tilt Stroke (PtV): 3.5 um
Actuator Pitch: 375 um
Pupil Size (Clear Aperture): 3.8 mm
Surface Quality (RMS): 40 nm

Deformable Mirrors: Precision Wavefront Control for Advanced Optical Systems

Deformable mirrors (DMs) are essential components in adaptive optics systems, enabling precise wavefront correction to compensate for optical aberrations. By dynamically adjusting their shape, DMs enhance image quality in various applications, from astronomy to biomedical imaging.

What Is a Deformable Mirror?

A deformable mirror is a reflective surface whose shape can be altered in real-time to correct wavefront distortions. These mirrors typically consist of a thin, flexible membrane supported by an array of actuators. The actuators adjust the mirror's surface to match the desired wavefront, compensating for aberrations introduced by factors like atmospheric turbulence or optical system imperfections.

Types of Deformable Mirrors

Deformable mirrors come in various designs, each suited to specific applications:

  • MEMS (Micro-Electro-Mechanical Systems) Mirrors: Utilize microfabricated actuators to achieve high-speed, high-precision wavefront control. MEMS mirrors are commonly used in applications requiring rapid response times, such as laser beam shaping and retinal imaging.

  • Piezoelectric Mirrors: Employ piezoelectric actuators that change shape when an electric field is applied. These mirrors offer high stroke and low hysteresis, making them ideal for applications like high-power laser systems and space telescopes.

  • Electromagnetic Mirrors: Use electromagnetic actuators to deform the mirror surface. These mirrors provide high stroke and are suitable for applications requiring large-scale wavefront correction.

  • Ferrofluid Mirrors: Feature a reflective liquid surface that changes shape when exposed to a magnetic field. Ferrofluid mirrors offer continuous surface deformation and are used in specialized applications like laser beam shaping.

Applications of Deformable Mirrors

Deformable mirrors are employed across various fields:

  • Astronomy: In ground-based telescopes, DMs correct for atmospheric distortions, enabling high-resolution imaging of celestial objects. Notable projects like the Gemini Planet Imager and the Daniel K. Inouye Solar Telescope utilize DMs to enhance image quality .

  • Biomedical Imaging: In ophthalmology and microscopy, DMs improve image resolution by compensating for ocular aberrations, facilitating detailed imaging of retinal structures .

  • Laser Systems: DMs are used to shape and stabilize laser beams in applications like laser machining, optical trapping, and laser communication.

  • Defense and Security: In high-powered laser systems, DMs correct for beam distortions, enhancing the effectiveness of directed energy weapons and laser communication systems.

Choosing the Right Deformable Mirror

Selecting an appropriate deformable mirror involves considering several factors:

  • Actuator Count: The number of actuators determines the mirror's ability to correct complex wavefronts. Higher actuator counts provide finer control over the mirror's shape.

  • Stroke: The maximum displacement of the actuators affects the mirror's ability to correct large aberrations. A higher stroke allows for compensation of more significant distortions.

  • Response Time: The speed at which the mirror can adjust its shape is crucial for applications involving dynamic aberrations. Faster response times are necessary for real-time correction.

  • Surface Quality: The mirror's surface quality impacts the precision of wavefront correction. High-quality surfaces ensure accurate deformation and minimal residual aberrations.

Explore Deformable Mirrors on FindLight

FindLight offers a comprehensive selection of deformable mirrors from leading manufacturers. Our platform allows you to filter products based on key specifications, ensuring you find the perfect match for your application. Whether you're working in astronomy, biomedical imaging, or laser systems, FindLight provides the tools you need to enhance your optical systems.

Did You know?

Adaptive optics is the most revolutionary technological breakthrough in astronomy since Galileo’s exploration of the skies 400 years ago. Modern adaptive optics are Micro-Electro-Mechanical (MEM) devices and may contain over 1000 individual little mirrors that can each piston to a different position with the aid of mechanical actuators. These devices can change their shape 1000’s of times a second. In astronomy they allow for distortion correction of starlight that travels millions of light years across the vacuum of space only to get distorted by our atmosphere in the last 150 miles before reaching Earth.