Using vector magnetograms of 40 active regions (ARs) of the maximum of
solar cycle 22, we calculated the imbalance rho(h) (over the AR area)
of the current helicity h(c) = B-z (del x B)(z) in the photosphere. I
n 82.5% of the cases the predominant current helicity was negative (rh
o(h) < 0) in the northern hemisphere and positive (rho(h) > 0) in the
southern hemisphere. Thus, the predominance of counter-clockwise (cloc
kwise) vortices in the northern (southern) hemisphere seems to be vali
d not only for unipolar spots with obvious Vortex structure (Hale, 192
7; Richardson, 1941; McIntosh, 1979; Ding, Hong, and Wang, 1987) but a
lso for ARs of different types. The forces of rotation of the Sun (Cor
iolis force and/or differential rotation) seem to take effect in the t
wisting of various magnetic structures.