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Proceedings Paper

Modelling the optical pathway of the Large Binocular Telescope
Author(s): Michael Böhm; Thomas Ruppel; Jörg-Uwe Pott; Oliver Sawodny; Tom Herbst; Martin Kürster
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Paper Abstract

We dynamically model the Large Binocular Telescopes optical path using a linear system approach. The model is derived from experiments conducted at the telescope. These experiments will be described and we will explain the possibilities and difficulties in extracting a simulation model from measured data. The model also incorporates disturbances, such as wind forces and single excitations induced by vibrating machinery. We will show, why it is necessary to measure structural vibrations at the LBT and why we follow a model based approach in estimating the mirror’s oscillatory motions. Some simulation results will be presented and compared to measured time series and a conclusion will be drawn. An outlook will be given on how the observer can be implemented.

Paper Details

Date Published: 25 September 2012
PDF: 8 pages
Proc. SPIE 8449, Modeling, Systems Engineering, and Project Management for Astronomy V, 844915 (25 September 2012); doi: 10.1117/12.926293
Show Author Affiliations
Michael Böhm, Univ. of Stuttgart (Germany)
Thomas Ruppel, Univ. of Stuttgart (Germany)
Jörg-Uwe Pott, Max Planck Institute for Astronomy (Germany)
Oliver Sawodny, Univ. of Stuttgart (Germany)
Tom Herbst, Max Planck Institute for Astronomy (Germany)
Martin Kürster, Max Planck Institute for Astronomy (Germany)


Published in SPIE Proceedings Vol. 8449:
Modeling, Systems Engineering, and Project Management for Astronomy V
George Z. Angeli; Philippe Dierickx, Editor(s)

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