Abstract
The years under report 1964–67 are noted by a rapid development of the theory of optics in general and astrometrical instruments in particular. This period was characterized by the application of a new method to the study of the quality of optical systems on the basis of frequency-contrast characteristics, etc. The method of control and adjustment of optical instruments improved considerably (1, 2).
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Mel’nikov, O.A. (1967). Commission des Instruments Astronomiques. In: Perek, L. (eds) Reports on Astronomy/Proceedings of the Thirteenth General Assembly Prague 1967. International Astronomical Union Transactions, vol 13B. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3476-0_4
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