In the context of the Large Binocular Telescope project, we present the results of force actuator calibrations performed on an adaptive secondary prototype called P45, a thin deformable glass with magnets glued onto its back. Electromagnetic actuators, controlled in a closed loop with a system of internal metrology based on capacitive sensors, continuously deform its shape to correct the distortions of the wavefront. Calibrations of the force actuators are needed because of the differences between driven forces and measured forces. We describe the calibration procedures and the results, obtained with errors of less than 1.5%
Planned instruments utilizing multi-object adaptive optics systems on the forthcoming extremely larg...
this paper we describe the procedure for the optical calibration of large size deformable mirrors, a...
Large (> 1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely...
The two 911mm-diameter adaptive secondary (AS) mirrors for the Large Binocular telescope (LBT) are c...
This dissertation describes the development, calibration, and testing of the adaptive optics system ...
Deformable mirrors (DMs) are electromechanical devices used in ground-based telescopes to compensate...
Refractive index variations in the earth's atmosphere cause wavefront aberrations and limit thereby ...
We present the results of a complete set of static and dynamic runs of the FEA model of the MMT adap...
It is attractive to integrate a large deformable mirror for adaptive optics into an astronomical tel...
International audienceSeveral telescopes include large Deformable Mirrors (DM) located directly insi...
International audienceSeveral telescopes include large Deformable Mirrors (DM) located directly insi...
Deformable mirrors (DMs) are electromechanical devices used in ground-based telescopes to compensate...
International audienceSeveral telescopes include large Deformable Mirrors (DM) located directly insi...
Large (>1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely ...
Large (>1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely ...
Planned instruments utilizing multi-object adaptive optics systems on the forthcoming extremely larg...
this paper we describe the procedure for the optical calibration of large size deformable mirrors, a...
Large (> 1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely...
The two 911mm-diameter adaptive secondary (AS) mirrors for the Large Binocular telescope (LBT) are c...
This dissertation describes the development, calibration, and testing of the adaptive optics system ...
Deformable mirrors (DMs) are electromechanical devices used in ground-based telescopes to compensate...
Refractive index variations in the earth's atmosphere cause wavefront aberrations and limit thereby ...
We present the results of a complete set of static and dynamic runs of the FEA model of the MMT adap...
It is attractive to integrate a large deformable mirror for adaptive optics into an astronomical tel...
International audienceSeveral telescopes include large Deformable Mirrors (DM) located directly insi...
International audienceSeveral telescopes include large Deformable Mirrors (DM) located directly insi...
Deformable mirrors (DMs) are electromechanical devices used in ground-based telescopes to compensate...
International audienceSeveral telescopes include large Deformable Mirrors (DM) located directly insi...
Large (>1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely ...
Large (>1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely ...
Planned instruments utilizing multi-object adaptive optics systems on the forthcoming extremely larg...
this paper we describe the procedure for the optical calibration of large size deformable mirrors, a...
Large (> 1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely...