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Atmospheric turbulence effects on astrometric determinations

Published online by Cambridge University Press:  14 August 2015

V. I. Ivanov*
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Irkutsk, USSR

Extract

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It is well known that the turbulent state of the atmosphere gives rise to fluctuations of the coefficient of light refraction. In astrometric observations these fluctuations produce the phenomenon of image motion which serves as the source of accidental errors of observations. The need for the study of the effect of atmospheric turbulence is documented in (G.Teleki, 1967) and others.

Type
Research Article
Copyright
Copyright © Reidel 1979 

References

Høg, E.: 1968, Zeitschrift für Astroph., 69, pp.313325.Google Scholar
Kolchinsky, I.G.: 1967, Optical instability of the Earth atmosphere from observations of stars. Kiev, “Naukova dumka”.Google Scholar
Kolchinsky, I.G.: 1973, Astrometriya i astrofizika, 20, pp. 1939.Google Scholar
Lambeck, K.: 1968, SAO special report, 269, pp. 127.Google Scholar
Tatarsky, V.I.: 1967, Propagation of waves in a turbulent atmosphere. M., “Nauka”.Google Scholar
Teleki, G.: 1967, Proceedings of the 17 Astron. Conf. USSR. L., “Nauka”, pp. 101106.Google Scholar
Zilitinkevich, S.S.: 1970, Atmosphere boundary layer dynamics. L., Gidrometeoizdat.Google Scholar