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Updated: Jun 8, 2026

Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
Linear quadratic Gaussian control of a deformable mirror adaptive optics system with time-delayed measurements
We developed a new control technique for adaptive optics telescopes to correct atmospheric turbulence. This method uses a predictive controller and delayed measurements to improve image clarity.
Area of Science:
- Astronomy and Astrophysics
- Optical Engineering
- Control Systems
Background:
- Atmospheric turbulence distorts astronomical images, limiting ground-based telescope resolution.
- Adaptive optics (AO) systems use deformable mirrors to correct these distortions in real-time.
Purpose of the Study:
- To present a novel control technique for ground-based deformable mirror AO telescopes.
- To compensate for optical wave-front phase distortion caused by atmospheric turbulence.
Main Methods:
- Design of a predictive linear quadratic Gaussian (LQG) controller.
- Utilizing time-delayed wave-front slope measurements from a Hartmann-type sensor.
- Generating commanded control voltages for mirror actuators.
Main Results:
- The proposed LQG controller effectively compensates for atmospheric phase distortion.
- The technique demonstrates precise control over the deformable mirror actuators.
- Improved correction of optical wave-front phase distortion was achieved.
Conclusions:
- The developed predictive LQG control technique enhances AO system performance for ground-based telescopes.
- This method offers a robust solution for mitigating atmospheric turbulence effects.
- The findings contribute to achieving higher resolution astronomical observations from Earth.
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