The atmospheric quality of astronomical seeing at several points in the USSR

Details The atmospheric quality of astronomical seeing at several points in the USSR The atmospheric quality of astronomical seeing at several points in the USSR

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..632s&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, May-June 1991, p. 632-638. In Russian.

Astronomy and Astrophysics

Astronomy

4

Astronomical Observatories, Astronomical Photometry, Seeing (Astronomy), U.S.S.R., Atmospheric Turbulence, Histograms, Telescopes

Scientific paper

Distributions are presented of zenith-reduced atmospheric seeing angle values derived from Polaris image motion photoelectric measurements at ten sites in the USSR. The most favorable statistics of atmospheric seeing were found at the Mt. Sanglok observatory in Tadzhikistan, which is superior to the best investigated sites in the world with the exception of the Mauna Kea observatory in Hawaii.

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