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    Data-driven subspace predictive control of adaptive optics for high-contrast imaging

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    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.
    Show allShow less
    Affiliation
    University of Arizona, Wyant College of Optical Science
    University of Arizona, Steward Observatory
    Issue Date
    2021
    Keywords
    adaptive optics
    coronagraph
    exoplanets
    high-contrast imaging
    spectroscopy
    
    Metadata
    Show full item record
    Publisher
    SPIE
    Citation
    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).
    Journal
    Journal of Astronomical Telescopes, Instruments, and Systems
    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 access
    ISSN
    2329-4124
    DOI
    10.1117/1.JATIS.7.2.029001
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.1117/1.JATIS.7.2.029001
    Scopus Count
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    UA Faculty Publications

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