Share Email Print
cover

Proceedings Paper

Synoptic Seeing Measurements At The University Of Hawaii 2.2m Telescope
Author(s): J. P. Henry; G. Cecil; B. Barnes; F. Cheigh; L. A. Thompson
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

The average seeing at the University of Hawaii 2.2 m telescope from 10 August 1985 to 9 January 1986 was 0.95 ± 0.02 arcsec full width at half-maximum at a wavelength of 0.70 pm. We believe that the dome makes substantial contributions to this average because the see-ing degrades with increasing temperature difference between a point near the primary mirror and the outside air. There is no significant dependence on wavelength (over the range 0.63-0.82 μm), wind direction, or time (over the interval covered to date). The data reported in this paper are the baseline against which we will assess the results of a long-term program of dome thermal balance improvements.

Paper Details

Date Published: 20 August 1986
PDF: 6 pages
Proc. SPIE 0628, Advanced Technology Optical Telescopes III, (20 August 1986); doi: 10.1117/12.963523
Show Author Affiliations
J. P. Henry, University of Hawaii (United States)
G. Cecil, University of Hawaii (United States)
B. Barnes, University of Hawaii (United States)
F. Cheigh, University of Hawaii (United States)
L. A. Thompson, University of Hawaii (United States)


Published in SPIE Proceedings Vol. 0628:
Advanced Technology Optical Telescopes III
Lawrence D. Barr, Editor(s)

© SPIE. Terms of Use
Back to Top