Real-time modal control implementation for adaptive optics
- 20 July 1998
- journal article
- Published by Optica Publishing Group in Applied Optics
- Vol. 37 (21) , 4586-4597
- https://doi.org/10.1364/ao.37.004586
Abstract
The electronics, computing hardware, and computing used to provide real-time modal control for a laser guide-star adaptive optics system are presented. This approach offers advantages in the control of unobserved modes, the elimination of unwanted modes (e.g., tip and tilt), and automatic handling of the case of low-resolution lens arrays. In our two-step modal implementation, the input vector of gradients is first decomposed into a Zernike polynomial mode by a least-squares estimate. The number of modes is assumed to be less than or equal to the number of actuators. The mode coefficients are then available for collection and analysis or for the application of modal weights. Thus the modal weights may be changed quickly without recalculating the full matrix. The control-loop integrators are at this point in the algorithm. To calculate the deformable-mirror drive signals, the mode coefficients are converted to the zonal signals by a matrix multiply. When the number of gradients measured is less than the number of actuators, the integration in the control loop will be done on the lower-resolution grid to avoid growth of unobserved modes. These low-resolution data will then be effectively interpolated to yield the deformable-mirror drive signals.Keywords
This publication has 3 references indexed in Scilit:
- Adaptive Optics for Astronomy: Principles, Performance, and ApplicationsAnnual Review of Astronomy and Astrophysics, 1993
- Wave-front interpretation with Zernike polynomialsApplied Optics, 1980
- Zernike polynomials and atmospheric turbulence*Journal of the Optical Society of America, 1976