-transparent.png){kind=logo}
We present a technique for controlling a ground-based deformable mirror adaptive optics telescope to compensate for optical wave-front phase distortion induced by a turbulent atmosphere. Specifically, a predictive linear quadratic Gaussian (LQG) controller is designed that generates commanded control voltages to the mirror actuators based on a set of time-delayed wave-front slope measurements from a Hartmann-type wave-front sensor.
| UI | MeSH Term | Description | Entries |
|---|
Related Publications
R N Paschall, and
D J Anderson
June 2009,
Journal of the Optical Society of America. A, Optics, image science, and vision,
R N Paschall, and
D J Anderson
March 2014,
Applied optics,
R N Paschall, and
D J Anderson
January 2009,
Journal of the Optical Society of America. A, Optics, image science, and vision,
R N Paschall, and
D J Anderson
April 2018,
Optics letters,
R N Paschall, and
D J Anderson
April 2006,
Applied optics,
R N Paschall, and
D J Anderson
July 2007,
Applied optics,
R N Paschall, and
D J Anderson
August 2017,
Applied optics,
R N Paschall, and
D J Anderson
July 2000,
Journal of the Optical Society of America. A, Optics, image science, and vision,
R N Paschall, and
D J Anderson
November 2008,
Optics letters,
R N Paschall, and
D J Anderson
May 2003,
Optics express,
