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Published April 2016 | Submitted + Published
Journal Article Open

Multi time-step wavefront reconstruction for tomographic adaptive-optics systems

Abstract

In tomographic adaptive-optics (AO) systems, errors due to tomographic wavefront reconstruction limit the performance and angular size of the scientific field of view (FoV), where AO correction is effective. We propose a multi time-step tomographic wavefront reconstruction method to reduce the tomographic error by using measurements from both the current and previous time steps simultaneously. We further outline the method to feed the reconstructor with both wind speed and direction of each turbulence layer. An end-to-end numerical simulation, assuming a multi-object AO (MOAO) system on a 30 m aperture telescope, shows that the multi time-step reconstruction increases the Strehl ratio (SR) over a scientific FoV of 10 arc min in diameter by a factor of 1.5–1.8 when compared to the classical tomographic reconstructor, depending on the guide star asterism and with perfect knowledge of wind speeds and directions. We also evaluate the multi time-step reconstruction method and the wind estimation method on the RAVEN demonstrator under laboratory setting conditions. The wind speeds and directions at multiple atmospheric layers are measured successfully in the laboratory experiment by our wind estimation method with errors below 2  ms^(−1). With these wind estimates, the multi time-step reconstructor increases the SR value by a factor of 1.2–1.5, which is consistent with a prediction from the end-to-end numerical simulation.

Additional Information

© 2016 Optical Society of America. Received 17 November 2015; revised 20 January 2016; accepted 28 January 2016; posted 11 February 2016 (Doc. ID 253736); published 22 March 2016. Funding: Japan Society for the Promotion of Science (JSPS) (15J02510, 23740140, 26287027); Agence Nationale de la Recherche (ANR) (ANR-11-IDEX-0001-02. Thanks to Naruhisha Takato, Yutaka Hayano, and Jean-Pierre Véran for many discussions. Thanks to the staff members of Subaru Telescope for their support. Y. Ono is supported by Japan Society for the Promotion of Science (JSPS) Grant-in-Aid for JSPS Fellows (15J02510). M. Akiyama is supported by JSPS Grant-in-Aid for Young Scientist (B) (23740140) and Grant-in-Aid for Scientific Research (B) (26287027). C. Correia is supported by Agence Nationale de la Recherche (ANR) (ANR-11-IDEX-0001-02).

Attached Files

Published - josaa-33-4-726.pdf

Submitted - 1604.02849v1.pdf

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Additional details

Created:
August 20, 2023
Modified:
October 18, 2023