Cycles of phase evolution of solar activity and cosmic-ray variations
are reconstructed by means of the delay component method, which allows
us to study the temporal behaviour of time lag between solar activity
and cosmic-ray cycle phases. It is shown that the period of the late
20th cycle was very unusual. We have found a delay in the phase of the
solar activity cycle with respect to that of cosmic rays and discuss
the heliospheric conditions responsible for this delay.