Abstract
Sunspot records in the seventeenth century provide important information on the solar activity before the Maunder minimum, yielding reliable sunspot indices and the solar butterfly diagram. Galilei’s letters to Cardinal Francesco Barberini and Marcus Welser contain daily solar observations on 3 – 11 May, 2 June – 8 July, and 19 – 21 August 1612. These historical archives do not provide the time of observation, which results in uncertainty in the sunspot coordinates. To obtain them, we present a method that minimizes the discrepancy between the sunspot latitudes. We provide areas and heliographic coordinates of 82 sunspot groups. In contrast to Sheiner’s butterfly diagram, we found only one sunspot group near the Equator. This provides a higher reliability of Galilei’s drawings. Large sunspot groups are found to emerge at the same longitude in the northern hemisphere from 3 May to 21 August, which indicates an active longitude.
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Acknowledgements
We thank the referee for the substantial revision and helpful comments. The reported study was partially funded by RFBR according to the research projects 15-02-06959-a and 16-02-00300-a.
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Figures 15, 16, 17, 18, 19, and 20 show sunspots sorted into groups. Black rectangles with numbers denote individual sunspots or subgroups of sunspots. Green ovals mark sunspot groups. Note that “not a sunspot” shows paper defects. For convenience, blue and pink lines represent the \(x\)-and \(y\)-axes in the rectangular coordinate system, and the solar limb is shown as a red circle. Note that on 14 June, one tiny spot is missing in the image provided by the Galileo Project; this spot was added by us for completeness.
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Vokhmyanin, M.V., Zolotova, N.V. Sunspot Positions and Areas from Observations by Galileo Galilei. Sol Phys 293, 31 (2018). https://doi.org/10.1007/s11207-018-1245-1
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DOI: https://doi.org/10.1007/s11207-018-1245-1