Paper
10 November 2011 Integrated model of the Carlina Telescope
Author Affiliations +
Proceedings Volume 8336, Integrated Modeling of Complex Optomechanical Systems; 83360J (2011) https://doi.org/10.1117/12.921015
Event: Integrated Modeling of Complex Optomechanical Systems, 2011, Kiruna, Sweden
Abstract
The Carlina hypertelescope is a planned sparse aperture 100 m telescope with pupil densification. The telescope has a spherical primary with segments located in a valley between mountains, and additional optical elements in a gondola suspended in eight cables some 100 m above the primary mirror. The resolution is about 1.2×10-3 arcsec. It is imperative that the position and attitude of the gondola be maintained within tight tolerances during observation and star tracking. The present design has servo-controlled winches on the ground for control of the gondola via the cables. An integrated model of the system, including optics, cables, gondola, position and attitude control system, and wind disturbances has been set up. The structural and control models are linear. Calculations in the frequency domain and simulations in the time domain show that the performance of the telescope with the present design seems adequate for short exposures. However, for long-exposure operation, the gondola stability should be improved by about two orders of magnitude. Recommendations are given on possible approaches for performance improvement.
© (2011) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Anita Enmark, Torben Andersen, Mette Owner-Petersen, Rijuparna Chakraborty, and Antoine Labeyrie "Integrated model of the Carlina Telescope", Proc. SPIE 8336, Integrated Modeling of Complex Optomechanical Systems, 83360J (10 November 2011); https://doi.org/10.1117/12.921015
Lens.org Logo
CITATIONS
Cited by 5 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Motion models

Monochromatic aberrations

Telescopes

Motion measurement

Point spread functions

Integrated modeling

Zemax

Back to Top