Sunspot group tilt angle measurements from historical observations
arXiv:1603.02510 · doi:10.1016/j.asr.2016.03.002
Abstract
Sunspot positions from various historical sets of solar drawings are analysed with respect to the tilt angles of bipolar sunspot groups. Data by Scheiner, Hevelius, Staudacher, Zucconi, Schwabe, and Spoerer deliver a series of average tilt angles spanning a period of 270 years, additional to previously found values for 20th-century data obtained by other authors. We find that the average tilt angles before the Maunder minimum were not significantly different from the modern values. However, the average tilt angles of a period 50 years after the Maunder minimum, namely for cycles 0 and 1, were much lower and near zero. The normal tilt angles before the Maunder minimum suggest that it was not abnormally low tilt angles which drove the solar cycle into a grand minimum.
accepted by Advances in Space Research
References in corpus (1)
Cited by in corpus (9)
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- A New Calibrated Sunspot Group Series Since 1749: Statistics of Active Day Fractions
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- Christian Horrebow's Sunspot Observations -- II. Construction of a Record of Sunspot Positions
- Nature of grand minima and maxima from fully non-linear Flux-Transport Dynamos
- Sunspot Drawings by Japanese Official Astronomers in 1749-1750
- Calibration of full-disk He I 10830 Å filtergrams of the Chromospheric Telescope
- Solar observatory Einstein Tower -- Data release of the digitized solar full-disk photographic plate archive