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Proceedings Paper

A possible concept for the day-time calibration and co-phasing of the adaptive M4 mirror at the E-ELT telescope
Author(s): Runa Briguglio; Giorgio Pariani; Marco Xompero; Armando Riccardi; Matteo Tintori; Daniele Gallieni; Roberto Biasi
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Paper Abstract

The M4 unit is the deformable mirror providing the E-ELT with adaptive correction of the atmospheric turbulence. The mirror is segmented into 6 petals which are actively shaped by more than 5000 voice-coil actuators. They are controlled in close loop with internal metrology through co-located capacitive position sensors. INAF is involved in the optical calibration and verification of the M4 unit and designed the laboratory optical testbed In this paper, we present a possible auxiliary setup for the mirror calibration once installed at the telescope. The concept implements an on-demand, day-time, optical re-calibration of the mirror, to ensure the years-long term, high accuracy, high precision stability of the internal metrology, beyond the already remarkable intrinsic electronic stability of the M4 unit. The setup exploits the two focii of the quasi-elliptical M3 to create an optical cavity, with the interferometer placed at a Nasmyth focal station of the ELT and a retroreflector (or fiber source) at the M3 short focus to measure the M4 in double (or single) pass. The full monitoring of the M4 optical area allows to: calibrate the actuator influence functions to compute the segments piston tip/tilt commands with high precision; retrieve the flattening command to correct from the low and high order features generated by thermo-mechanical and electrical drifts; compute the phasing command to correct for the segments differential alignment and piston within the requested WF accuracy. The system offers a fast and effective optical maintenance facility for the M4U, without requiring an additional test tower and the mount/dismount down-time of the unit. In this work, we summarize the optical layout and the flattening and segments co-phasing strategy.

Paper Details

Date Published: 18 July 2018
PDF: 8 pages
Proc. SPIE 10703, Adaptive Optics Systems VI, 1070379 (18 July 2018); doi: 10.1117/12.2314460
Show Author Affiliations
Runa Briguglio, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Giorgio Pariani, INAF - Osservatorio Astronomico di Brera (Italy)
Marco Xompero, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Armando Riccardi, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Matteo Tintori, ADS International (Italy)
Daniele Gallieni, ADS International (Italy)
Roberto Biasi, Microgate (Italy)


Published in SPIE Proceedings Vol. 10703:
Adaptive Optics Systems VI
Laird M. Close; Laura Schreiber; Dirk Schmidt, Editor(s)

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