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Extreme Adaptive Optics

Optics seminar by Olivier Guyon, Steward Observatory; University of Arizona

Hosted by PSW Science

Friday 20:00 New York (GMT-5)

Recording available

Online

Recording

Abstract

Olivier Guyon explains the physics and engineering of extreme adaptive optics for directly imaging exoplanets. Atmospheric turbulence distorts incoming wavefronts; sensors measure those distortions and deformable mirrors apply compensating corrections. The lecture covers guide stars, fast detectors, actuators, real-time computing and control systems. Extreme adaptive optics requires correction rates above a kilohertz, mirrors with more than a thousand actuators and nanometer-scale measurements of optical aberrations. Guyon describes how integrated systems suppress and calibrate unwanted starlight, including approaches developed with the Subaru Extreme Adaptive Optics system. These advances support efforts to equip extremely large telescopes to image potentially habitable planets.

Topics

extreme adaptive opticsAtmospheric turbulencedeformable mirrorsguide starsfast detectorsreal-time computingSubaru Extreme Adaptive Optics

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