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A&A 365, 314-323 (2001)
DOI: 10.1051/0004-6361:20000185
Piston control with adaptive optics in stellar interferometry
Application to the GI2T interferometer and bimorph mirrors
C. Vérinaud1 and F. Cassaing2 .1 Observatoire de la Côte d'Azur (OCA), Département Fresnel, 2130, route de l'Observatoire, 06460 Saint-Vallier-de-Thiey, France
2 Office National d'Études et de Recherches Aérospatiales (ONERA), DOTA, BP 72, 92322 Châtillon Cedex, France
(Received 29 August 2000 / Accepted 18 October 2000)
Abstract
The general purpose of an adaptive optics system is to
correct for the wavefront corrugations due to atmospheric turbulence. When
applied to a stellar interferometer, care must be taken in the control of the
mean optical path length, commonly called differential piston. This paper
defines a general formalism for the piston control of a deformable mirror in
the linear regime. It is shown that the usual filtering of the piston mode in
the command space is not sufficient, mostly in the case of a bimorph mirror.
Another algorithm is proposed to cancel in the command space the piston
produced in the pupil space. This analysis is confirmed by simulations in the
case of the GI2T interferometer located on Plateau de Calern, France. The
contrast of the interference fringes is severely reduced in the case of a
classical wavefront correction, even in short exposures, but is negligible
with our algorithm, assuming a realistic calibration of the mirror. For this
purpose, a simple concept for the calibration of the piston induced by a
deformable mirror is proposed.
Key words: instrumentation: interferometers -instrumentation: adaptive optics - atmospheric effects -methods: numerical -techniques: interferometric
Offprint request: C. Vérinaud
© ESO 2001
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