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
Lens.org Logo
CITATIONS
Cited by 4 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Cameras

Mirrors

Telescopes

Finite element methods

Phase modulation

Large Synoptic Survey Telescope

Shape memory alloys

RELATED CONTENT

LSST secondary mirror assembly baseline design
Proceedings of SPIE (September 17 2012)
Gemini near-infrared imager (NIRI)
Proceedings of SPIE (August 16 2000)
Seismic analysis of the LSST telescope
Proceedings of SPIE (September 17 2012)
Aluminium-based high-resolution camera for a small satellite
Proceedings of SPIE (November 15 2002)

Back to Top