tween, could be ignored. Then the tripod was moved consecutively to the floats 5, 4, 3 and 2, and the respective micrometer readings registered together with those of the corresponding settings of the interference pattern in the laser line. The sequence was concluded by readings at the terminal no. I again. After a proportional reduction for the dif ferences between the readings at this terminal the intermediate readings may be compared with the settings of the micrometer as calculated by inter polation. The differences A would show at least the order of magnitude of the influence of the vertical refraction. The intermediate readings were the mean of two series of 10 settings each. The s.d. can be estimated as 1.6 pm (inclusive the s.d. of the standardization) so that the s.d. of a difference A would amount to 1.9 pm. Four examples are given below, the first one show ing the method of calculation, the last one showing the largest difference A ever obtained. (Rounded off to pm). part of this influence by the inclusion of a liquid level surface as a reference. One can measure the vertical distance of two fixed terminal points of the alignment in respect of this surface, calculate the position of intermediate points by interpolation and set the micrometer accordingly. The instrumentation required is complex, but may be justified for specific purposes. The instrumentation described is only experimental and can of course be perfected for use in practice. A eknowledgements The high precision instruments were built in the workshop of the Department by Messrs. D. A. de Wit and D. Joghems with exceptional skill. The electronics was designed and built on specification by the Technical and Physical Engineering Services at Wageningen. 9 7 4 Conclusion From the results it may be inferrred that the vertical long term refraction has a more considerable influence on an alignment than would be expected at first sight. It seems possible to eliminate the larger float 1 2 3 4 5 6 1st example readings 7985 9054 7972 8196 8426 8637 8824 interp. for time* 13 10 8 5 3 0 reduced read. 7985 8206 8434 8642 8827 9054 earth curv. 0 1 2 5 8 13 correct, read. 7985 8205 8432 8637 8819 9041 calcul. interp. 7985 8196 8407 8619 8830 9041 differences A urn 0 +25 18 -11 0 2nd example differences Aum 0 15 - 4 15 0 3rd example differences A;j.m 0 16 18 +26 - 6 0 4th example differences Ap.m 0 35 14 +48 19 0 infl. of evapor., temp. etc. References Anon., 1948. Precision of telescope pointing. J. Coast and Geodetic Survey no. I Geilen, Q., 1971. Untersuchungen zur Richtungsstabilitat von HeNe-Lasern mit Hilfe von Elektronischen Messlatten. Veröff. Geodat. Inst. T.H. Aachen no. 19. Van Heel, A. C. S., 1950. High precision measurements with simple equipment. J. Opt. Soc. Am. Vol. 40, nr. 12, p. 809-816. Jensen, H., 1950. Formulas for the astronomical correction to precise levelling. Bull. Geodésique no. 17, p. 267-277. Oostenrijk, G., 1968. Het nieuwe meerpunts precisie waterpas „De Nivelmatic". Tijdschr. Kadaster Landmeetkunde (84) no. 4, p. 212-238. Richardus, P., 1963. The application of diffractive light in Surveying. Ph.D. dissertation. Richardus, P., 1968. Richten en Inrichten. Tijdschr. Kadaster en Landmeetkunde (84) no. 6, p. 415—427. Sneddon, J., 1974. Temperature effects in hydrostatic lev elling. Survey Review no. 174 p. 361-374. Sneddon, J., 1975. Hydrostatic methods of precise levelling. Ph.D. dissertation, The University of New South Wales. Waalewijn, A., 1964. Hydrostatic levelling in the Netherlands. Survey Review no. 131, p. 212-221; no. 132, p. 267-276. Washer, F. E. and Williams, H. B., 1946. Precision of tele scope pointing for outdoor targets. J. Opt. Soc. Am. 36. Washer, F. E., 1947. Effect of magnification on the precision of outdoor telescope pointing. J. Research (U.S.). Bureau of Standards 39. ngt 76 141

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