Abstract
In the framework of power-model of the structure function, the tropospheric limitations of accuracy of coordinate measurements, using phase and fringe frequency are shown. The general formulae, numerical estimates and a comparison between absolute and differential methods are given. It is shown that the tropospheric limitations are especially considerable for coordinate measurements, using fringe frequency.
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Dravskikh, A.F., Finkelstein, A.M. Tropospheric limitations in phase and frequency coordinate measurements in astronomy. Astrophys Space Sci 60, 251–265 (1979). https://doi.org/10.1007/BF00644330
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DOI: https://doi.org/10.1007/BF00644330