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• W3100230817 abstract "The sunspot drawings of Johann Staudacher of 1749–1799 were used to determine the solar differential rotation in that period. These drawings of the full disk lack any indication of their orientation. We used a Bayesian estimator to obtain the position angles of the drawings, the corresponding heliographic spot positions, a time offset between the drawings and the differential rotation parameter δΩ, assuming the equatorial rotation period is the same as today. The drawings are grouped in pairs, and the resulting marginal distributions for δΩ were multiplied. We obtain δΩ = −0.048 ± 0.025 d-1 (−2.75 °/d) for the entire period. There is no significant difference to the value of the present Sun. We find an (insignificant) indication for a change of δΩ throughout the observing period from strong differential rotation, δΩ ≈ −0.07 d-1, to weaker differential rotation, δΩ ≈ −0.04 d-1." @default.
• W3100230817 created "2020-11-23" @default.
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• W3100230817 date "2012-06-20" @default.
• W3100230817 modified "2023-09-23" @default.
• W3100230817 title "The solar differential rotation in the 18th century" @default.
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• W3100230817 doi "https://doi.org/10.1051/0004-6361/201219266" @default.
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