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Calibrating the interaction matrix for the LINC-NIRVANA high layer wavefront sensor.

作者信息

Zhang Xianyu, Arcidiacono Carmelo, Conrad Albert R, Herbst Thomas M, Gaessler Wolfgang, Bertram Thomas, Ragazzoni Roberto, Schreiber Laura, Diolaiti Emiliano, Kuerster Martin, Bizenberger Peter, Meschke Daniel, Rix Hans-Walter, Rao Changhui, Mohr Lars, Briegel Florian, Kittmann Frank, Berwein Juergen, Trowitzsch Jan

机构信息

Max Planck Institute for Astronomy, Koenigstuhl 17, D-69117 Heidelberg,Germany.

出版信息

Opt Express. 2012 Mar 26;20(7):8078-92. doi: 10.1364/OE.20.008078.

Abstract

LINC-NIRVANA is a near-infrared Fizeau interferometric imager that will operate at the Large Binocular Telescope. In preparation for the commissioning of this instrument, we conducted experiments for calibrating the high-layer wavefront sensor of the layer-oriented multi-conjugate adaptive optics system. For calibrating the multi-pyramid wavefront sensor, four light sources were used to simulate guide stars. Using this setup, we developed the push-pull method for calibrating the interaction matrix. The benefits of this method over the traditional push-only method are quantified, and also the effects of varying the number of push-pull frames over which aberrations are averaged is reported. Finally, we discuss a method for measuring mis-conjugation between the deformable mirror and the wavefront sensor, and the proper positioning of the wavefront sensor detector with respect to the four pupil positions.

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