  Longitudinal distributions of the photospheric magnetic field studied on the
base of National Solar Observatory (Kitt Peak) data (1976 - 2003) displayed two
opposite patterns during different parts of the 11-year solar cycle.
Heliolongitudinal distributions differed for the ascending phase and the
maximum of the solar cycle on one hand, and for the descending phase and the
minimum on the other, depicting maxima around two opposite Carrington
longitudes (180 deg. and 0/360 deg.). Thus the maximum of the distribution
shifted its position by 180 deg. with the transition from one characteristic
period to the other. Two characteristic periods correspond to different
situations occurring in the 22-year magnetic cycle of the Sun, in the course of
which both global magnetic field and the magnetic field of the leading sunspot
in a group change their sign. During the ascending phase and the maximum
(active longitude 180 deg.) polarities of the global magnetic field and those
of the leading sunspots coincide, whereas for the descending phase and the
minimum (active longitude 0/360 deg.) the polarities are opposite. Thus the
observed change of active longitudes may be connected with the polarity changes
of Sun's magnetic field in the course of 22-year magnetic cycle.
