  The vector representation of sunspots is used to study the nonaxisymmetric
features of the solar activity distribution (sunspot data from Greenwich -
USAF/NOAA, 1874 - 2016).The vector of the longitudinal asymmetry is defined for
each Carrington rotation; its modulus characterizes the magnitude of the
asymmetry, while its phase points to the active longitude. These
characteristics are to a large extent free from the influence of a stochastic
component and emphasize the deviations from the axisymmetry. For the sunspot
area, the modulus of the vector of the longitudinal asymmetry changes with the
11-year period; however, in contrast to the solar activity, the amplitudes of
the asymmetry cycles obey a special scheme. Each pair of cycles from 12 to 23
follows in turn the Gnevyshev - Ohl rule (an even solar cycle is lower than the
following odd cycle) or the anti-Gnevyshev - Ohl rule (an odd solar cycle is
lower than the preceding even cycle). This effect is observed in the
longitudinal asymmetry of the whole disk and the southern hemisphere. Possibly,
this effect is a manifestation of the 44-year structure in the activity of the
Sun. Northern hemisphere follows the Gnevyshev - Ohl rule in Solar Cycles 12 -
17, while in Cycles 18 - 23 the anti-rule is observed.
