Paper
10 July 2008 Wind induced image degradation (jitter) of the LSST telescope
Author Affiliations +
Abstract
A wind pressures PSD measured on the Gemini South Telescope was applied to the FEA model of the LSST telescope to determine the RMS motions of the principal optical systems. These motions were then converted to the time domain. The time domain motions were analyzed in the ZEMAX® software to determine the wind induced image degradation. This degradation was shown to be tolerable.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Douglas R. Neill, Jacques Sebag, Michael Warner, and Victor Krabbendam "Wind induced image degradation (jitter) of the LSST telescope", Proc. SPIE 7012, Ground-based and Airborne Telescopes II, 70120W (10 July 2008); https://doi.org/10.1117/12.790025
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Cited by 4 scholarly publications.
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KEYWORDS
Cameras

Mirrors

Telescopes

Finite element methods

Phase modulation

Large Synoptic Survey Telescope

Shape memory alloys

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