Results 181 to 190 of about 5,696 (229)
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Wavefront correction based on a reflective liquid crystal wavefront sensor
Journal of Optics A: Pure and Applied Optics, 2008A novel wavefront sensor (WFS) based on liquid crystal on silicon (LCOS) is demonstrated. The design of the liquid crystal microlens array with LCOS is given in detail. To save the energy of the incident light, an optimized optical design of the WFS is also considered.
L Hu +7 more
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High-speed Holographic Wavefront Correction
Imaging and Applied Optics 2016, 2016We present details of a compact, holographic adaptive optics system with 64 actuators and 100kHz bandwidth, but no computer. We are currently modifying our system with a view towards an on-sky test in a large astronomical telescope in late-2016.
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Aperture size effect on ultrasonic wavefront distortion correction
IEEE Transactions on Ultrasonics, Ferroelectrics and Frequency Control, 2004The influences of aperture size on wavefront distortion correction are investigated both theoretically and numerically. A multilayer, phase-screen model is assumed to be the underlying, distorting medium. Numerical simulations were performed using three wavefront distortion correction methods: time-shift compensation (TSC), backpropagation followed by ...
Deng-Huei, Huang, Jenho, Tsao
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Monolithic piezoelectric mirror for wavefront correction
Applied Physics Letters, 1974Experimental and theoretical analysis show that a spatially varying potential applied to one surface of a thick block of piezoelectric material will induce a piezoelectric deformation of that surface proportional to the potential at each point of the surface.
J. Feinleib, S. G. Lipson, P. F. Cone
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Wavefront correction inside unbalanced nulling interferometer
SPIE Proceedings, 2012In an unbalanced nulling interferometer (UNI) of our coronagraph system, the incidence light is divided into two, and they interfere by a reverse phase with different amplitude. Thereby, phase errors are magnified and we can correct a wavefront with higher precision.
Masaaki Horie +9 more
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Tomagraphic wavefront correction for the LSST
SPIE Proceedings, 2006The Large Synoptic Survey Telescope (LSST) is a three mirror modified Paul-Baker design with an 8.4m primary, a 3.4m secondary, and a 5.0m tertiary followed by a 3-element refractive corrector producing a 3.5 degree field of view. This design produces image diameters of
Phillion, D. W. +4 more
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Wavefront correction through image sharpness maximisation
SPIE Proceedings, 2005A key component of any adaptive optics system (AO) for the correction of wavefront aberrations, is the wavefront sensor(WFS). Many systems operate in a mode where a WFS measures the aberrations present in the incoming beam. The required corrections are determined and applied by the wavefront corrector - often a deformable mirror (DM).
L. P. Murray, J. C. Dainty, E. Daly
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Correction of large amplitude wavefront aberrations
SPIE Proceedings, 2005Recently, a number of research groups around the world have developed ophthalmic instruments capable of in vivo diffraction limited imaging of the human retina. Adaptive optics was used in these systems to compensate for the optical aberrations of the eye and provide high contrast, high resolution images. Such compensation uses a wavefront sensor and a
S. A. Cornelissen +5 more
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Wavefront correction by liquid-crystal devices
Soviet Journal of Quantum Electronics, 1986An experimental investigation was made of the use of liquid-crystal phase correctors of wavefronts. Prototype correctors were prepared with independent addressing of the elements and these were found capable of compensating distortions of wavefronts of radiation of wavelengths 0.5–6μ.
A A Vasil'ev +2 more
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Fundamentals of Ocular Wavefront Correction
2009For vision correction, the key is to help patients achieve good visual performance. In most cases, this means good visual acuity and good contrast sensitivity. The ocular aberrations can be considered as a combination of the spherocylindrical aberrations and irregular aberrations.
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