This paper reports the results of a study of the N-S asymmetry in the
flare index using the results of Knoska (1985) combined with our resul
ts for the solar cycles 17 to the current cycle 22. By comparing the t
ime-variation of the asymmetry curve with the solar activity variation
of the 11-year cycle, we have found that the flare index asymmetry cu
rve is not in phase with the solar cycle and that the asymmetry peaks
during solar minimum. A periodic behaviour in the N-S asymmetry appear
s: the activity in one hemisphere is more important during the ascendi
ng part of the cycle whereas during the descending part the activity b
ecomes more important in the other hemisphere. The dominance of flare
activity in the southern hemisphere continues during cycle 22 and, acc
ording to our findings, this dominance will increase gradually during
the following cycle 23.