Cycle Dependence of Hemispheric Activity
M. Temmer (1),
A. Veronig (1),
J. Rybák (2),
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
Data of daily hemispheric Sunspot numbers are analyzed including the time
span 1975-2001.
The study of north-south asymmetries concerning solar activity and rotational
behaviors is in particular relevant, as it is related to the solar dynamo and
the generation of magnetic fields.
As diagnostic tools we use wavelets and autocorrelation functions in
combination with statistical significance tests that are applied separately
for the to the northern and southern hemisphere.
Pronounced differences between the northern hemisphere shows a rigid rotation
of ~27 days which can be followed up to 15 periods in the autocorrelation
function.
The signal of the southern hemisphere is strongly attenuated after 3
recurrences showing variable periods in the range ~26-28.5 days.
The presence of these periods is not permanent during a cycle suggesting
activity pulses in each hemisphere.
For the northern hemisphere strong relations to the motion of deeper lying
convective structures building up long-living 'active zones' are suggested.
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