We have examined the more than 1100 drawings of the solar disk made by the German astronomy amateur Johann Caspar Staudach during 1749-1799 and counted the spots on each image. Using the modern perception of how to group spots into active regions we regrouped the spots as a modern observer would. The resulting number of groups was found to be on average 25 % higher than the first count of groups performed by Wolf in 1857, and used by Hoyt and Schatten in their construction of the Group Sunspot Number. Compared to other observers at the time, Staudach’s drawings have a very low average number, ~2, of spots per group, possibly indicating an inferior telescope likely suffering from spherical and chromatic aberration as would typical of amateur...
Sunspot observations are available in fairly good numbers since 1610, after the invention of the tel...
The focus of this study is to reveal the reason behind a scale problem detected around 1849 in the h...
The International Sunspot Number is used as a measure of the level of solar activity in many importa...
Jean Tarde and Jan Smogulecki carried out sunspot observations in the 1610s and 1620s at the dawn of...
Samuel Heinrich Schwabe made 8486 drawings of the solar disc with sunspots in the period from 1825 N...
Aims. Sunspot number series are composed from observations of hundreds of different observers that r...
Aims. Digital images of observations printed in the books Rosa Ursina sive solis and Prodromus pro s...
Aims. Extending the knowledge about the properties of solar cycles into the past is essential for un...
Aims. Sunspot number series are composed from observations of hundreds of different observers that r...
Abstract. In the one hundred years since Wolf died, little effort has gone into research to see if i...
Aims. Sunspot numbers form a benchmark series in many studies, but may still contain inhomogeneities...
Abstract Context: The group sunspot number (GSN) series constitute the longest instrumental astronom...
Abstract. At the XIIth Hvar Astrophysical Colloquium in 2012, we reviewed the progress of an effort ...
The sunspot number is “arguably the most intensively studied time series in astrophysics ” [Charbonn...
The Maunder Minimum (MM), which occurred between 1645 and 1715, is mainly known as an almost spotles...
Sunspot observations are available in fairly good numbers since 1610, after the invention of the tel...
The focus of this study is to reveal the reason behind a scale problem detected around 1849 in the h...
The International Sunspot Number is used as a measure of the level of solar activity in many importa...
Jean Tarde and Jan Smogulecki carried out sunspot observations in the 1610s and 1620s at the dawn of...
Samuel Heinrich Schwabe made 8486 drawings of the solar disc with sunspots in the period from 1825 N...
Aims. Sunspot number series are composed from observations of hundreds of different observers that r...
Aims. Digital images of observations printed in the books Rosa Ursina sive solis and Prodromus pro s...
Aims. Extending the knowledge about the properties of solar cycles into the past is essential for un...
Aims. Sunspot number series are composed from observations of hundreds of different observers that r...
Abstract. In the one hundred years since Wolf died, little effort has gone into research to see if i...
Aims. Sunspot numbers form a benchmark series in many studies, but may still contain inhomogeneities...
Abstract Context: The group sunspot number (GSN) series constitute the longest instrumental astronom...
Abstract. At the XIIth Hvar Astrophysical Colloquium in 2012, we reviewed the progress of an effort ...
The sunspot number is “arguably the most intensively studied time series in astrophysics ” [Charbonn...
The Maunder Minimum (MM), which occurred between 1645 and 1715, is mainly known as an almost spotles...
Sunspot observations are available in fairly good numbers since 1610, after the invention of the tel...
The focus of this study is to reveal the reason behind a scale problem detected around 1849 in the h...
The International Sunspot Number is used as a measure of the level of solar activity in many importa...