2019
DOI: 10.1029/2018sw002147
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Eric Strach: Four Decades of Detailed Synoptic Solar Observations (1969‐2008)

Abstract: Eric H. Strach (1914‐2011) studied medicine at University of Prague and graduated in 1938. Strach dedicated a great part of his life to astronomy becoming a consistent and meticulous observer. He joined the Liverpool Astronomical Association and British Astronomical Association during the 1960s and obtained two recognitions as proof of his great work in solar physics: the BAA's Merlin Medal and Gift in 1999 and Walter Goodacre Medal and Gift, 10 years later. Strach recorded four decades (1969‐2008) of systemat… Show more

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Cited by 5 publications
(3 citation statements)
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“…Further, recent revisions of sunspot number based on historical documents require us to re-evaluate the solar activity for a longer time span (Clette and Lefevre, 2016;Vaquero et al, 2016). Thaddäus Derfflinger's sunspot observations during 1802-1824, The Astrophysical Journal, doi: 10.3847/1538-4357/ab65c9 et al, 2007Arlt, 2008Arlt, , 2009Arlt, , 2018Hayakawa et al, 2018aHayakawa et al, , 2018bCarrasco et al, 2015Carrasco et al, , 2016Carrasco et al, , 2018Carrasco et al, , 2019bDenig and McVaugh, 2017), remove apparent continuous spotless days (Vaquero, 2007;Vaquero et al, 2016), and revise observations based on modern viewpoints (Vaquero et al, 2016;Svalgaard, 2017;Hayakawa et al, 2018d;Arlt et al, 2013Arlt et al, , 2016Fujiyama et al, 2019;Karoff et al, 2019;Jørgensen et al, 2019;Pevtsov et al 2019). Based on these revisions, a long-term variation of solar activity was evaluated utilising multiple methodologies (Svalgaard and Schatten, 2016;Usoskin et al, 2016;Clette and Lefevre, 2016;Chatzistergos et al, 2017).…”
Section: Introductionmentioning
confidence: 99%
“…Further, recent revisions of sunspot number based on historical documents require us to re-evaluate the solar activity for a longer time span (Clette and Lefevre, 2016;Vaquero et al, 2016). Thaddäus Derfflinger's sunspot observations during 1802-1824, The Astrophysical Journal, doi: 10.3847/1538-4357/ab65c9 et al, 2007Arlt, 2008Arlt, , 2009Arlt, , 2018Hayakawa et al, 2018aHayakawa et al, , 2018bCarrasco et al, 2015Carrasco et al, , 2016Carrasco et al, , 2018Carrasco et al, , 2019bDenig and McVaugh, 2017), remove apparent continuous spotless days (Vaquero, 2007;Vaquero et al, 2016), and revise observations based on modern viewpoints (Vaquero et al, 2016;Svalgaard, 2017;Hayakawa et al, 2018d;Arlt et al, 2013Arlt et al, , 2016Fujiyama et al, 2019;Karoff et al, 2019;Jørgensen et al, 2019;Pevtsov et al 2019). Based on these revisions, a long-term variation of solar activity was evaluated utilising multiple methodologies (Svalgaard and Schatten, 2016;Usoskin et al, 2016;Clette and Lefevre, 2016;Chatzistergos et al, 2017).…”
Section: Introductionmentioning
confidence: 99%
“…While observations were conducted over many decades in various institutional observatories such as Greenwich (Willis et al, 2013(Willis et al, , 2016a(Willis et al, , 2016b, Debrecen (Baranyi et al, 2016;Győri et al, 2017), or Mount Wilson (Lefèvre et al, 2005Pevtsov et al, 2019), long-term observations at smaller observatories by individual astronomers -frequently skilled amateur observers -are of particular importance in terms of stability. Indeed, such sunspot time series have been derived from a single observer, often with a unique telescope, in contrast with professional teams working in shifts and with a staff changing over the years (e.g., Clette et al, 2014;Carrasco et al, 2019).…”
mentioning
confidence: 99%
“…In fact, data from individual sunspot observers have played significant roles on calibrations of the International Sunspot Number (version 2; hereafter SILSO SN V2) and comparison with other solar-activity indices, with significant homogeneity (Mathieu et al, 2019;Clette, 2021). Recent efforts have examined and described some cases of individual sunspot observers (Carrasco et al, 2019;Clette et al, 2014;Hayakawa et al, 2020;Vaquero et al, 2016), whereas further available records have to be analysed in this context.…”
Section: Introductionmentioning
confidence: 99%