Sunspot Observations in 1684-1702: John Flamsteed and Philippe de La Hire
Nadezhda Zolotova, Mikhail Vokhmyanin
TL;DR
The paper reconstitutes sunspot activity during the Maunder Minimum by systematically curating and reanalyzing Flamsteed and La Hire observations (1684–1702), including drawings and engravings from Cassini and contemporaries. Using VSOP87-based ephemerides and pixel-weighted solar coordinates, the authors reconstruct sunspot positions, areas, latitudes, and group tracks, and estimate sidereal rotation rates from both nearby-day and long-interval methods. The results reveal sunspot latitudes clustered around roughly -10°, rotation rates near 14.0–14.5° per day, and a tendency for Joy's law to be obeyed rather than violated, with notable activity nests and occasional discrepancies due to instrument and orientation effects. The study highlights the value of historical records for calibrating long-term solar indices and for informing models of differential rotation and the solar-cycle behavior during grand minima, while providing openly accessible, digitized data for future work.
Abstract
In this work, we present an extensive review and detailed analysis of sunspot measurements, drawings, and engravings made by John Flamsteed and, mainly, by Philippe de La Hire during the Maunder minimum. All available information and contemporary knowledge about the sunspot nature are shown. The coordinates, areas, and numbers of sunspots and sunspot groups are reconstructed. Based on these observations, La Hire, Jean-Dominique Cassini, and his son Jacques Cassini regularly published results that shed light on the purpose of sunspot measurements and the scientific paradigm of that time. In particular, astronomers believed that sunspots were recurrent over decades. We compare the reconstructed time-latitude diagram with those obtained by Spoerer (Ueber die periodicitat der sonnenflecken seit dem Jahre 1618..., 1889) and Ribes and Nesme-Ribes (Astron. Astrophys. 276, 549, 1993). The sidereal differential rotation rate is estimated, and its latitudinal profile is reconstructed. We also evaluate the fraction of sunspot groups that obey or violate Joy's law.
