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The first experience of solar eclipse observations with a miniature torsion balance

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Abstract

We observed the behavior of the pointer of an asymmetric torsion balance (TB) at solar eclipse dates and on other off-eclipse days. A peculiar reaction of the miniature TB different from its reaction at off-eclipse time was recorded for some solar eclipses. The relative positions of the Earth, Moon, and Sun are among the possible factors affecting the position of the TB pointer. A time shift between the maximum phase of a solar eclipse and the maximum TB reaction was detected. We conclude that base observations of such phenomena from different points of the terrestrial globe are necessary.

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Original Russian Text © A.F. Pugach, M.M. Medvedskii, N.N. Peretyatko, V.I. Shavlovskii, V.L. Karbovskii, T.V. Nikityuk, P.F. Lazorenko, A.V. Zolotukhina, D.P. Vorobyev, V.A. Pap, G.A. Lazorenko, I.P. Vedenicheva, S.V. Shatokhina, N.M. Kostogryz, 2008, published in Kinematika i Fizika Nebesnykh Tel, 2008, Vol. 24, No. 5, pp. 401–410.

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Pugach, A.F., Medvedskii, M.M., Peretyatko, N.N. et al. The first experience of solar eclipse observations with a miniature torsion balance. Kinemat. Phys. Celest. Bodies 24, 253–258 (2008). https://doi.org/10.3103/S088459130805005X

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  • DOI: https://doi.org/10.3103/S088459130805005X

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