Merging Two Data Sets of Hemispheric Sunspot Numbers
J. Rybák (1),
P. Bendik (1),
M. Temmer (2),
A. Veronig (2),
A. Hanslmeier (2)
1 - Astronomical Institute, Slovak Academy of Sciences, SK-05960 Tatranská Lomnica, Slovakia
2 - Institut for Geophysics, Astrophysics and Meteorology, Universitätsplatz 5, A-8010 Graz, Austria
First results on merging two data sets of hemispheric sunspot
numbers - from the Kanzelhohe Solar Observatory and
the Skalnate Pleso Observatory - for the time span
1977-1978 are presented. A total coverage of
86% was reached for the merged data set. In order to have a
homogeneous time series, the daily sunspot numbers for the full
disk from both observing stations were normalized to the
international relative sunspot number of the day. The
derived hemispheric sunspot numbers from Kanzelhohe and
Skalnate Pleso Observatory compared for 290 common observing
show very high correlations (r>=0.95), and
the estimated data noise yields significant differences only for
small values of sunspot numbers. These outcomes demonstrate the high potential
of the applied merging procedure, and are the basis for an ongoing
project to derive hemispheric sunspot numbers back to the year
1945 using sunspot drawings from Kanzelhohe and Skalnate
Pleso Observatory.
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