Hemispheric Sunspot Numbers Rn and Rs
from 1945-2004: Catalogue and N-S asymmetry analysis for solar cycles
18-23
M. Temmer (1),
J. Rybák (2),
P. Bendik (2),
A. Veronig (1),
F. Vogler (1),
W. Otruba (1),
W. Potzi (1),
A. Hanslmeier (1)
1 - Institut for Geophysics, Astrophysics and Meteorology, Universitätsplatz 5, A-8010 Graz, Austria
2 - Astronomical Institute, Slovak Academy of Sciences, SK-05960 Tatranská Lomnica, Slovakia
Astronomy & Astrophysics 447, 735-743 (2006)
A&A paper: PDF file
Catalogue data:
Readme file,
Monthly Rn and Rs data file,
Daily Rn and Rs data file (compressed - gz)
ABSTRACT:From sunspot drawings provided by the Kanzelhohe Solar Observatory, Austria,
and the Skalnate Pleso Observatory, Slovak Republic, we extracted a data
catalogue of hemispheric Sunspot Numbers covering the time span 1945-2004.
The validated catalogue includes daily, monthly-mean, and smoothed-monthly
relative sunspot numbers for the northern and southern hemispheres separately
and is available for scientific use. These data we then investigated with
respect to north-south asymmetries for almost 6 entire solar cycles
(Nos. 18-23). For all the cycles studied, we found that the asymmetry
based on the absolute asymmetry index is enhanced near the cycle maximum,
which contradicts to previous results that are based on the normalized
asymmetry index. Moreover, the weak magnetic interdependence between the
two solar hemispheres is confirmed by their self-contained evolution during
a cycle. For the time span 1945-2004, we found that the cycle maxima and
also the declining and increasing phases are clearly shifted, whereas the
minima seem to be in phase for both hemispheres. The asymmetric behavior
reveals no obvious connection to either the sunspot cycle period
of ~11- or the magnetic cycle of ~22-years. The most
striking excess of activity is observed for the northern hemisphere
in cycles 19 and 20.