Center for Adaptive Optics
IntroductionAdaptive OpticsResearchEducation/HRMembersMeetings
PublicationsSoftwareEmploymentSearch CfAOLinksWhat's New
CfAO Newsletters

Center for
Adaptive Optics
Volume 2

Download PDF

In this Volume:

Sharper Image with Adaptive Optics

Low Cost Wavefront Correctors for Vision Science Adaptive Optics

Creating and Detecting Rayleigh Laser Guide Stars

People and Profiles

From the Director

Year 2 - NSF Site Visit a week after Sept 11

First Light for Keck Laser Guide Star

Astronomers Observe Distant Galaxies More Clearly

Education and Human Resource Activities

Education and Human Resources Notices

Upcoming AO Related Conferences

CfAO visits the USAF's Advanced Electro-Optical System site at Maui and Gemini Observatory – January 2002.

Low Cost Wavefront Correctors for Vision Science Adaptive Optics

Nathan Doble and David Williams - Center for Visual Science, University of Rochester

Adaptive optics (AO) for astronomy has been an established discipline for a couple of decades. The last five or so years has seen successful application of this technology to imaging the human eye. Current vision AO systems have generally used the low volume, high cost AO components found on telescopes. The mirrors alone are expensive ($1000 per channel), physically large and lack the necessary stroke required for correcting the aberrations of many eyes.Through CfAO, a collaboration is underway between the University of Rochester, Lawrence Livermore National Laboratory (LLNL), BostonMicroMachines Corporation (BMC), UC Berkeley and Lucent Technologies to investigate alternative low cost wavefront correctors for the next generation of ophthalmic instrumentation.

Various mirror designs are being explored but for a commercial instrument the mirror would need a corrective range greater than 1um, require over 100 channels and be small, ideally comparable to the pupil diameter (7mm). As a first step, a BMC MEMS mirror has been incorporated into the current Rochester AO testbed and a system containing a Hamamatsu liquid crystal spatial light modulator (LC-SLM) has been built by LLNL for delivery to UC Davis.

The BMC MEMS mirror: 144 actuators defined under a 3.3mm2 active area with a mirror stroke of 2um. Photograph BMC.

MEMS technology is appealing because the devices are very small (see comparison to the dime above) and would eventually allow high volume, low cost manufacture. One area that needs further development is the mirror stroke. Several CfAO groups have designs for higher stroke devices, including Lucent and UC Berkeley. The BSAC team at Berkeley has a segmented mirror design with over 10um of stroke operating at a low voltage (70-80 volts).

Initial results with the BMC MEMS have been very promising. For the first time, the AO loop was closed with a MEMS device instead of a conventional mirror. The results before and after correction are shown for a subject with a 4.6mm pupil.

Before and after AO results for a 4.6mm pupil with the BMC MEMS mirror as the corrective element

The system built by LLNL for UC Davis uses an optically addressed Liquid Crystal Spatial Light Modulator (LC-SLM) to provide the wavefront correction. It avoids the need for large stroke due to the fact that it is segmented and can be phase wrapped. A photo of the UC Davis system is shown at right. The LC-SLM can be seen in the back right of the breadboard.

A low cost AO system for vision science would be very useful in earlier diagnosis and monitoring of treatments for many retinal diseases. In addition, such a system could be used as a means of showing patients the benefits of a vision correction procedure, such as LASIK or contact lenses. The ongoing research described here will eventually lead to several prototype AO equipped phoropters. These devices will be tested at several CfAO nodes with a view to commercialization.
The Liquid Crystal Spatial Light Modula-tor (LC-SLM) AO system designed by LLNL for delivery to UC Davis. Photo-graph Scot Olivier, LLNL

Design Copyright © 2002 University of California Regents