Stochastic optimization for adaptive real -time wavefront correction

We have investigated the performance of an adaptive optics system subjected to changing atmospheric conditions, under the guidance of the ALOPEX stochastic optimization. Atmospheric distortions are smoothed out by means of a deformable mirror, the shape of which can be altered in order to follow the...

Descripción completa

Detalles Bibliográficos
Autores: Zakynthinaki, M. S., Saridakis, Yannis. G.
Tipo de recurso: artículo
Fecha de publicación:2002
País:España
Institución:Universitat Politècnica de Catalunya (UPC)
Repositorio:UPCommons. Portal del coneixement obert de la UPC
Idioma:inglés
OAI Identifier:oai:upcommons.upc.edu:2117/878
Acceso en línea:https://hdl.handle.net/2117/878
Access Level:acceso abierto
Palabra clave:Electromagnetic theory
Mathematical programming
Stochastic optimization
ALOPEX algorithm
Adaptive wavefront correction
Zernike polynomials
Deformable mirror
Masking
Òptica
Electromagnetisme
Programació (Matemàtica)
Classificació AMS::90 Operations research, mathematical programming::90C Mathematical programming
Classificació AMS::78 Optics, electromagnetic theory::78M Basic methods
Descripción
Sumario:We have investigated the performance of an adaptive optics system subjected to changing atmospheric conditions, under the guidance of the ALOPEX stochastic optimization. Atmospheric distortions are smoothed out by means of a deformable mirror, the shape of which can be altered in order to follow the rapidly changing atmospheric phase fluctuations. In a simulation model, the total intensity of the light measured on a central area of the image (masking area) is used as the cost function for our stochastic optimization algorithm, while the surface of the deformable mirror is approximated by a Zernike polynomial expansion. Atmospheric turbulence is simulated by a number of Kolmogorov filters. The method's effectiveness, that is its ability to follow the motion of the turbulent wavefronts, is studied in detail and as it pertains to the size of the mirror's masking area, to the number of Zernike polynomials used and to the degree of the algorithm's stochasticity in relation to the mean rate of change of atmospheric distortions. Computer simulations and a series of numerical experiments are reported to show the successful implementation of the method.