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


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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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M. Murzabekov

All-Russian Research Institute of Physical

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Email: murzabekov@vniiftri.ru
俄罗斯联邦, Mendeleevo, Moscow oblast, 141570

V. Fateev

All-Russian Research Institute of Physical

Email: murzabekov@vniiftri.ru
俄罗斯联邦, Mendeleevo, Moscow oblast, 141570

A. Pruglo

All-Russian Research Institute of Physical

Email: murzabekov@vniiftri.ru
俄罗斯联邦, Mendeleevo, Moscow oblast, 141570

S. Ravdin

All-Russian Research Institute of Physical

Email: murzabekov@vniiftri.ru
俄罗斯联邦, Mendeleevo, Moscow oblast, 141570

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