J. W. Pastorff of Drossen, Germany, made about 1477 observations of su
nspots between 1819 and 1833. These observations were erroneously inte
rpreted by A. C. Ranyard in 1874 and then used by Rudolf Wolf in his c
alculations of the Wolf Sunspot Numbers. The result is a noisier daily
time series and overestimation of the monthly and yearly means for th
ese years. Pastorff was actually a very good observer. In this paper,
Pastorff's original observations are reexamined and more nearly correc
t values for the number of sunspot groups are tabulated. We show some
examples of the problems created by Ranyard's interpretation and the c
onsequences for the history of solar activity that a correct interpret
ation of Pastorff's observations will have. Pastorff's observations pr
ovide valuable information on the first strong cycle after the Dalton
Minimum (1795-1823).