Sunspots during the Maunder Minimum from Machina Coelestis by Hevelius
arXiv:1502.06270 · doi:10.1007/s11207-015-0767-z
Abstract
We revisited the sunspot observations published by Johannes Hevelius in his book Machina Coelestis (1679) corresponding to the period 1653-1675 (just in the middle of the Maunder Minimum). We show detailed translations of the original Latin texts describing the sunspot records and provide the general context of these sunspot observations. From this source only, we present an estimate of the annual values of the Group Sunspot Number based only on the records that explicitly inform about the presence or absence of sunspots. Although we obtain very low values of the Group Sunspot Number, in accordance with a grand minimum of solar activity, these values are significantly higher in general than the values provided by Hoyt and Schatten (1998) for the same period.
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Cited by in corpus (21)
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- A Great Space Weather Event in February 1730
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- Strong evidence of low levels of solar activity during the Maunder Minimum
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- Iwahashi Zenbei's Sunspot Drawings in 1793 in Japan
- Revisiting Kunitomo's Sunspot Drawings during 1835-1836 in Japan
- Intense geomagnetic storm during Maunder minimum possibly by a quiescent filament eruption
- The Celestial Sign in the Anglo-Saxon Chronicle in the 770s: Insights on Contemporary Solar Activity
- Sunspot observations by Charles Malapert during the period 1618-1626: a key dataset to understand solar activity before the Maunder minimum
- Revisiting the Amplitude of Solar Cycle 9: The Case of Sunspot Observations by W.C. Bond
- On the use of naked-eye sunspot observations during the Maunder Minimum
- Could a Hexagonal Sunspot Have Been Observed During the Maunder Minimum?
- A Transit of Venus Possibly Misinterpreted as an Unaided-Eye Sunspot Observation in China on 9 December 1874
- Long-lived sunspots in historical records: a case study analysis from 1660 to 1676
- Sunspot Observations in 1684-1702: John Flamsteed and Philippe de La Hire