Paper
1 July 1990 Seeing measurements at the Multiple Mirror Telescope obtained with a very high quality 1.8-m primary mirror
Frederic H. Chaffee, Richard H. Cromwell
Author Affiliations +
Abstract
Image-quality data are presented which were gathered at the University of Arizona's Multiple Mirror Telescope (MMT) using a very high quality 1.8-m mirror, for median image sizes of 0.72 arcsec in 8-sec integrations. The measured image is judged to have been degraded by 0.48 arcsec from that allowed by the free atmosphere by such factors as errors in telescope focus, collimation, mirror support, mirror seeing, and the combined optical figure of the five mirror surfaces required to bring the light to the image-analysis CCD. These data imply the appropriateness of a total optical error budget of 0.2 arcsec for 8-m diameter telescopes currently being designed.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Frederic H. Chaffee and Richard H. Cromwell "Seeing measurements at the Multiple Mirror Telescope obtained with a very high quality 1.8-m primary mirror", Proc. SPIE 1236, Advanced Technology Optical Telescopes IV, (1 July 1990); https://doi.org/10.1117/12.19167
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Cited by 2 scholarly publications.
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KEYWORDS
Mirrors

Telescopes

Image quality

Video

Atmospheric optics

Stars

Cameras

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