Data-driven subspace predictive control of adaptive optics for high-contrast imaging
Author
Haffert, S.Y.Males, J.R.
Close, L.M.
Van Gorkom, K.
Long, J.D.
Hedglen, A.D.
Guyon, O.
Schatz, L.
Kautz, M.
Lumbres, J.
Rodack, A.
Knight, J.M.
Sun, H.
Fogarty, K.
Affiliation
University of Arizona, Wyant College of Optical ScienceUniversity of Arizona, Steward Observatory
Issue Date
2021
Metadata
Show full item recordPublisher
SPIECitation
Haffert, S. Y., Males, J. R., Close, L. M., Van Gorkom, K., Long, J. D., Hedglen, A. D., Guyon, O., Schatz, L., Kautz, M., Lumbres, J., Rodack, A., Knight, J. M., Sun, H., & Fogarty, K. (2021). Data-driven subspace predictive control of adaptive optics for high-contrast imaging. Journal of Astronomical Telescopes, Instruments, and Systems, 7(2).Rights
Copyright © 2021 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The search for exoplanets is pushing adaptive optics (AO) systems on ground-based telescopes to their limits. One of the major limitations at small angular separations, exactly where exoplanets are predicted to be, is the servo-lag of the AO systems. The servo-lag error can be reduced with predictive control where the control is based on the future state of the atmospheric disturbance. We propose to use a linear data-driven integral predictive controller based on subspace methods that are updated in real time. The new controller only uses the measured wavefront errors and the changes in the deformable mirror commands, which allows for closed-loop operation without requiring pseudo-open loop reconstruction. This enables operation with non-linear wavefront sensors such as the pyramid wavefront sensor. We show that the proposed controller performs near-optimal control in simulations for both stationary and non-stationary disturbances and that we are able to gain several orders of magnitude in raw contrast. The algorithm has been demonstrated in the lab with MagAO-X, where we gain more than two orders of magnitude in contrast. © 2021 Society of Photo-Optical Instrumentation Engineers (SPIE).Note
Immediate accessISSN
2329-4124Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/1.JATIS.7.2.029001