2020
DOI: 10.1007/s41116-020-0023-y
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Historical sunspot records

Abstract: Sunspot observations are available in fairly good numbers since 1610, after the invention of the telescope. This review is concerned with those sunspot observations of which longer records and drawings in particular are available. Those records bear information beyond the classical sunspot numbers or group sunspot numbers. We begin with a brief summary on naked-eye sunspot observations, in particular those with drawings. They are followed by the records of drawings from 1610 to about 1900. The review is not a … Show more

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Cited by 103 publications
(63 citation statements)
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“…Following the onset of sunspot observations in 1610 (e.g., Clette et al, 2014;Arlt & Vaquero, 2020), similar prolonged solar minima have been identified in cosmogenic isotope data based on long-term enhancements of 14 C and 10 Be (e.g., Usoskin, 2017; see Table 1). Major prolonged solar minima over the past millennium gained notoriety in solar physics following a series of studies in the 1970s and 1980s.…”
Section: Naming Of the Grand Minima And The Dalton Minimumsupporting
confidence: 60%
“…Following the onset of sunspot observations in 1610 (e.g., Clette et al, 2014;Arlt & Vaquero, 2020), similar prolonged solar minima have been identified in cosmogenic isotope data based on long-term enhancements of 14 C and 10 Be (e.g., Usoskin, 2017; see Table 1). Major prolonged solar minima over the past millennium gained notoriety in solar physics following a series of studies in the 1970s and 1980s.…”
Section: Naming Of the Grand Minima And The Dalton Minimumsupporting
confidence: 60%
“…Naked-eye sunspot observations are the only direct information on historical activity from historical documents of the last two millennia (Arlt & Vaquero, 2020). Fortunately, there are various catalogues of this kind of observations available in the scientific literature (Wittmann & Xu, 1987;Yau & Stephenson, 1988).…”
Section: Datamentioning
confidence: 99%
“…While such a long phase coherence, observed in two rather unrelated proxy datasets for the Schwabe cycle, is most remarkably in itself, one might be even more puzzled by the almost complete equivalence of the cycle period of 11.04 years with the corresponding 11.07‐year period as derived for the last centuries (Stefani et al 2019, 2020). Ironically, the latter value for the more recent times is more disputable than the value for the early Holocene given that the systematic observation of sunspots goes back only to the times of Scheiner and Galileo (Arlt & Vaquero 2020), with grave uncertainties for the time of the Maunder minimum (1645–1715).…”
Section: Introductionmentioning
confidence: 99%