The cause of discrepancy between astroclimatic prognosis and the real quality of imaging in large telescopes

Details The cause of discrepancy between astroclimatic prognosis and the real quality of imaging in large telescopes The cause of discrepancy between astroclimatic prognosis and the real quality of imaging in large telescopes

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...93n&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Mar.-Apr. 1989, p. 93-96. In Russian.

Mathematics

Logic

Ambient Temperature, Astronomical Observatories, Meteorological Parameters, Telescopes, Climatology, Domes, Optical Transfer Function, U.S.S.R.

Scientific paper

The discrepancy between astroclimatic prognosis and the real quality of imaging in large telescopes at most observatories is explained mainly by the imperfect temperature regime inside and outside of the dome. The use of the optical transfer function method provides a quantitative estimate of the effect of the dome's influence on the size of the stellar image in the telescope.

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