Paper
10 February 2006 Analysis of secondary mirror mold topography to Large Millimeter Telescope using fringe projection technique
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Proceedings Volume 6046, Fifth Symposium Optics in Industry; 60461X (2006) https://doi.org/10.1117/12.674606
Event: Fifth Symposium Optics in Industry, 2005, Santiago De Queretaro, Mexico
Abstract
The Large Millimeter Telescope (LMT)1 is a 50 m diameter millimeter-wave telescope designed for principal operation at wavelengths between 1mm and 4mm. The LMT secondary mirror will have a diameter of approximately 2.6 meters and focal ratio of .35. The purpose of this study was to implement the incoherent fringe projection technique and the spatial phase synchronous method to measure the secondary mirror mold profiling. The obtained topography is compared with the conic surface generated synthetically. We considered that mold should be hyperboloid surface with paraxial curvature of 1764.9 mm and conic constant of -1.1474. We will discuss the preliminary results where it is obtained a RMS of 0.624 cm.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Amalia Martínez, J. A. Rayas, Sergio Vázquez, and Alberto Jaramillo "Analysis of secondary mirror mold topography to Large Millimeter Telescope using fringe projection technique", Proc. SPIE 6046, Fifth Symposium Optics in Industry, 60461X (10 February 2006); https://doi.org/10.1117/12.674606
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KEYWORDS
Mirrors

Fringe analysis

Telescopes

Profiling

3D acquisition

CCD cameras

Image processing

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