Computationally efficient, practical implementation of tomographic minimum variance wavefront control using laser and natural guide stars for multi-conjugate adaptive optics

Minimum variance tomographic wavefront reconstruction is described in the literature as a 2-step process consisting of the estimation of dominant layers of distributed turbulence above the telescope, followed by least-squares fitting of this estimate onto deformable mirrors (DMs). The estimation problem is performed from wavefront sensor (WFS) measurements obtained from multiple guide stars. For many science cases, laser guide stars (LGSs) are required to increase sky coverage, but in this case a small number of low-order modes of the LGS WFS measurements are strongly corrupted by the uncertain position of the LGS on the sky and must be projected out from the range space of the turbulence-to-LGS WFS influence matrix. These modes are the global tip and tilt (TT) modes for each LGS WFS and possibly the differential focus modes between LGS WFSs. One possible approach to sense these null modes is to incorporate low-order natural guide star (NGS) WFS measurements in the estimation problem, although this complicates the practical implementation of the reconstruction algorithms. To overcome such complication, a split LGS/NGS wavefront control architecture has recently been proposed for multi-conjugate adaptive optics (MCAO). Such an architecture implements two separate control loops driven independently by the closed-loop LGS and NGS measurements, with distinct wavefront reconstruction algorithms and temporal filters applied to the LGS- and NGS-controlled modes. Control of the NGS modes is now a low dimensional problem, so that the reconstruction algorithm and servo bandwidth can be rapidly updated when the NGS asterism or the atmospheric conditions change. Sample simulation results illustrating the comparative performance of the integrated and split approaches are reviewed. Finally, a split Zernike-based architecture for multi-object adaptive optics (MOAO) is discussed.

[1]  Jean-Christophe Sinquin,et al.  Progress toward developing the TMT adaptive optical systems and their components , 2008, Astronomical Telescopes + Instrumentation.

[2]  T. Fusco,et al.  ELP-OA: status report of the setup of the demonstrator of the Polychromatic Laser Guide Star at Observatoire de Haute-Provence , 2010 .

[3]  APPENDIX 4.6.B EFFICIENT COMPUTATION OF MINIMUM VARIANCE WAVEFRONT RECONSTRUCTORS USING SPARSE MATRIX TECHNIQUES , 2002 .

[4]  Brent L. Ellerbroek,et al.  Simulations of closed-loop wavefront reconstruction for multiconjugate adaptive optics on giant telescopes , 2003, SPIE Optics + Photonics.

[5]  B L Ellerbroek,et al.  Constrained matched filtering for extended dynamic range and improved noise rejection for Shack-Hartmann wavefront sensing. , 2008, Optics letters.

[6]  Brent L Ellerbroek,et al.  Efficient computation of minimum-variance wave-front reconstructors with sparse matrix techniques. , 2002, Journal of the Optical Society of America. A, Optics, image science, and vision.

[7]  Luc Gilles,et al.  Wavefront error budget development for the Thirty Meter Telescope laser guide star adaptive optics system , 2008, Astronomical Telescopes + Instrumentation.

[8]  Francois Rigaut,et al.  Laser guide star in adaptive optics : the tilt determination problem , 1992 .

[9]  Onera,et al.  The FALCON concept: multi-object spectroscopy combined with MCAO in near-IR , 2001, astro-ph/0109289.

[10]  F. Rigaut,et al.  Methods for correcting tilt anisoplanatism in laser-guide-star-based multiconjugate adaptive optics. , 2001, Journal of the Optical Society of America. A, Optics, image science, and vision.

[11]  Luc Gilles,et al.  Progress towards developing the TMT adaptive optical systems and their components , 2008 .

[12]  Jacques M. Beckers,et al.  Increasing the size of the isoplanatic patch with multiconjugate adaptive optics. , 1988 .

[13]  Luc Gilles,et al.  Closed-loop stability and performance analysis of least-squares and minimum-variance control algorithms for multiconjugate adaptive optics. , 2005, Applied optics.

[14]  B. Ellerbroek,et al.  Split atmospheric tomography using laser and natural guide stars. , 2008, Journal of the Optical Society of America. A, Optics, image science, and vision.