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A Method for Correcting for Tilt Errors in a Plumb-Line Deviation Astrometer

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Abstract

An improved method for measuring the deviation from the normal to the geoid using a digital telescope is presented. The algorithm for the traditional method is described together with the algorithms and performance characteristics of the proposed method. This paper is based on a presentation made at the conference “Modern Astrometry 2017,” dedicated to the memory of K.V. Kuimov (Sternberg Astronomical Institute, Moscow State University, October 23–25, 2017).

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Authors and Affiliations

  1. All-Russian Research Institute of Physical, Technical, and Radio Technical Measurements, Mendeleevo, Moscow oblast, 141570, Russia

    M. M. Murzabekov, V. F. Fateev, A. V. Pruglo & S. S. Ravdin

Authors
  1. M. M. Murzabekov
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  2. V. F. Fateev
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  3. A. V. Pruglo
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  4. S. S. Ravdin
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Corresponding author

Correspondence to M. M. Murzabekov.

Additional information

Original Russian Text © M.M. Murzabekov, V.F. Fateev, A.V. Pruglo, S.S. Ravdin, 2018, published in Astronomicheskii Zhurnal, 2018, Vol. 95, No. 12, pp. 912–914.

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Murzabekov, M.M., Fateev, V.F., Pruglo, A.V. et al. A Method for Correcting for Tilt Errors in a Plumb-Line Deviation Astrometer. Astron. Rep. 62, 1013–1015 (2018). https://doi.org/10.1134/S1063772918120107

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  • DOI: https://doi.org/10.1134/S1063772918120107

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