Paper
27 July 2016 Dimensioning the MAORY real time computer
Author Affiliations +
Abstract
The MAORY system is the Multi-Adaptive Optics module for the European Extremely Large Telescope first light. MAORY should provide high and homogeneous image quality over the MICADO Field of View (about 1 arcmin diameter) and still an acceptable correction up to the 3 arcmin technical Field of View. The baseline of MAORY is therefore to rely upon the use of multiple Laser Guide Stars (6), multiple Natural Guide Stars (3) and multiple Deformable Mirrors correction. The Real-Time Computer is a key sub-system of MAORY. It must collect the measurements from various sensing devices and drive thousands of actuators. Many correction loops are foreseen with different update rates. The main requirements concerning the system dimensioning and Real-Rime performance depend on the sensors and on the actuators interface and on the Real-Time Data Processing. In this paper we give a preliminary description of the MAORY Real-Time Control system functional requirements derived from the system baseline at the beginning of the instrument Phase B.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Laura Schreiber, Emiliano Diolaiti, Carmelo Arcidiacono, Andrea Baruffolo, Giovanni Bregoli, Enrico Cascone, Giuseppe Cosentino, Simone Esposito, Corrado Felini, Italo Foppiani, Paolo Ciliegi, Philippe Feautrier, and Paolo Torroni "Dimensioning the MAORY real time computer", Proc. SPIE 9909, Adaptive Optics Systems V, 99094L (27 July 2016); https://doi.org/10.1117/12.2231527
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Cited by 3 scholarly publications.
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KEYWORDS
Telescopes

Real-time computing

Sensors

Wavefront sensors

Actuators

Mirrors

Control systems

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