Bošković's Spherical Trigonometric Solution for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 1777
arXiv:2507.20383 · doi:10.1007/s11207-025-02497-x
Abstract
In September 1777 Ruđer Bošković observed and measured the sun-spot positions to determine the solar rotation elements. In 1785, among other methods, he described a trigonometric spherical solution for the determination of the position of the axis and rate of the solar rotation using three sunspot positions, but without equations. For the first time, we derive the equations that are applicable to modern computers for calculating the solar rotation elements, as they were described by Bošković. We recalculated Bošković's original example using his measurements of sunspot positions from 1777 and the equations developed here, confirming his results from 1785. Bošković's methodology of arithmetic means determines , , and sidereal period separately, while the planar trigonometric solution determines and together. His spherical trigonometric solution calculates , , and the sidereal period in a single procedure. Keywords: Ruđer Bošković, Sunspots, Solar rotation, Spherical trigonometry
The article is the submitted one to the publisher upon the Licence to Publish by Springer Nature. Since its submission to acceptance, section 4.4. Accuracy Versus Precision of the Measurements on the Apparent Solar Disk, is added, the old section 4.4 became 4.5, and some references are added. Editor-in-Chief copy-edited the article. Published article is https://doi.org/10.1007/s11207-025-02497-x
References in corpus (4)
- Determination of the Solar Rotation Elements and Period from Ruđer Bošković's Sunspot Observations in 1777
- Bošković's method for determining the axis and rate of solar rotation by observing sunspots in 1777
- On the Determination of the Solar Rotation Elements i, Ω and Period using Sunspot Observations by Ruđer Bošković in 1777
- Solar rotation elements and period determined using sunspot observations by Ruđer Bošković in 1777