Paper
4 November 1982 10 m Telescope For Submillimeter Waves
Jacob W. M. Baars
Author Affiliations +
Abstract
This paper summarizes the salient features of a telescope for the sub-mm wavelength region, which we have begun to design. Operating from a high and dry mountain the telescope will be used for astronomical observations in the atmospheric transmission windows between 350 μm and 3 mm wavelength. The surface accuracy will be ≤ 15 μm, the reflector diameter ≈ 10 m and the pointing accuracy 1". Extensive use of graphite epoxy material shall eliminate thermal deformations.
© (1982) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jacob W. M. Baars "10 m Telescope For Submillimeter Waves", Proc. SPIE 0332, Advanced Technology Optical Telescopes I, (4 November 1982); https://doi.org/10.1117/12.933546
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KEYWORDS
Telescopes

Reflectors

Astronomy

Optical instrument design

Observatories

Astronomical telescopes

Extremely high frequency

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