Abstract
Systematic trends in the semi-diameter of the Sun from measurements made with the Cape Observatory transit circle in 1834 and from 1861 to 1871 and 1884 to 1892 (the only years for which raw observations of the solar limbs were available to us) should probably be attributed to large variations in the personal equation of the individual observers rather than to any real variation of the solar diameter.
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References
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© 1982 D. Reidel Publishing Company
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Smith, C., Messina, D. (1982). The Effect of Personal Equation on Measurements of the Solar Semi-Diameter by Transit Circle Observers. In: Fricke, W., Teleki, G. (eds) Sun and Planetary System. Astrophysics and Space Science Library, vol 96. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7846-1_8
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DOI: https://doi.org/10.1007/978-94-009-7846-1_8
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