Vibration environment of the LBTO/AO system

Pedro Escárate; Julian C. Christou; Gustavo Rahmer; John M. Hill; Doug L. Miller; Greg Taylor

doi:10.1117/12.2313882

18 July 2018 Vibration environment of the LBTO/AO system

Pedro Escárate, Julian C. Christou, Gustavo Rahmer, John M. Hill, Doug L. Miller, Greg Taylor

Author Affiliations +

Proceedings Volume 10703, Adaptive Optics Systems VI; 107034F (2018) https://doi.org/10.1117/12.2313882
Event: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States

Abstract

The majority of current Adaptive Optics (AO) systems do not compensate properly for vibrations within the optical path. For this reason the mitigation of vibration effects in astronomical AO systems is extremely important. The mechanical vibration effects, acting in the science light propagation path, strongly affect the performance of the LBTO/AO system. A frequency-based analysis of the pyramidal wavefront sensor data (PWFS) and the accelerometers network data (OVMS+) on the telescope structure was done in order to identify the principal mechanical vibration frequencies.

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Pedro Escárate, Julian C. Christou, Gustavo Rahmer, John M. Hill, Doug L. Miller, and Greg Taylor "Vibration environment of the LBTO/AO system", Proc. SPIE 10703, Adaptive Optics Systems VI, 107034F (18 July 2018); https://doi.org/10.1117/12.2313882

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