Deformable mirrors are used for changing the wavefront of the reflected light by using one or more actuators behind the mirror to physically deform it. This application is widely used in telescopes to compensate for atmospheric aberrations using a feedback wavefront sensor. Recent advances in lithography process require more precise wavefront control than ever, and deformable mirrors are being considered as a suitable optical unit in the optical column of lithography systems. Using electrostrictive materials for the actuation provides benefits like less hysteresis, no creep, and fast response time. One major limiting factor in the use of such materials is the high sensitivity of strain response to temperature. Due to application constraints...
Adaptive Optics is an essential technology in today's large telescopes to compensate for atmospheric...
Very large, light weight mirrors are being developed for applications in space. Due to launch mass a...
The resolution of ground-based telescopes is limited by the blurring caused by Earth’s turbulent atm...
It is attractive to integrate a large deformable mirror for adaptive optics into an astronomical tel...
International audienceACMAS program, in partnership with CNES and DGA, intends to develop an innovat...
In the production of integrated circuits (e.g. computer chips), optical lithography is used to trans...
The testing of a lightweight unimorph-type deformable mirror (DM) for wavefront correction in cryoge...
In a collaboration of the Technische Universiteit Eindhoven, Delft University of Technology and TNO ...
The electromechanical deformation of viscoelastic dielectric elastomers (DEs) is primarily governed ...
Under an applied voltage, dielectric elastomers (DEs) produce an actuation strain that is nonlinear,...
Large aperture and light weight space telescopes requires adaptive optics with deformable mirrors ca...
AbstractUnder an applied voltage, dielectric elastomers (DEs) produce an actuation strain that is no...
Deformable mirrors can be used in cryogenic instruments to compensate for temperature-induced deform...
The resolving power of an optical system is often limited by the presence of timevarying wavefront d...
[[abstract]]In this work, a fabrication and temperature compensation analysis and electrowetting for...
Adaptive Optics is an essential technology in today's large telescopes to compensate for atmospheric...
Very large, light weight mirrors are being developed for applications in space. Due to launch mass a...
The resolution of ground-based telescopes is limited by the blurring caused by Earth’s turbulent atm...
It is attractive to integrate a large deformable mirror for adaptive optics into an astronomical tel...
International audienceACMAS program, in partnership with CNES and DGA, intends to develop an innovat...
In the production of integrated circuits (e.g. computer chips), optical lithography is used to trans...
The testing of a lightweight unimorph-type deformable mirror (DM) for wavefront correction in cryoge...
In a collaboration of the Technische Universiteit Eindhoven, Delft University of Technology and TNO ...
The electromechanical deformation of viscoelastic dielectric elastomers (DEs) is primarily governed ...
Under an applied voltage, dielectric elastomers (DEs) produce an actuation strain that is nonlinear,...
Large aperture and light weight space telescopes requires adaptive optics with deformable mirrors ca...
AbstractUnder an applied voltage, dielectric elastomers (DEs) produce an actuation strain that is no...
Deformable mirrors can be used in cryogenic instruments to compensate for temperature-induced deform...
The resolving power of an optical system is often limited by the presence of timevarying wavefront d...
[[abstract]]In this work, a fabrication and temperature compensation analysis and electrowetting for...
Adaptive Optics is an essential technology in today's large telescopes to compensate for atmospheric...
Very large, light weight mirrors are being developed for applications in space. Due to launch mass a...
The resolution of ground-based telescopes is limited by the blurring caused by Earth’s turbulent atm...