  It was as early as the 1980s that A V Gurevich and his group proposed a
theory to explain the magnetosphere of radio pulsars and the mechanism by which
they produce coherent radio emission. The theory has been sharply criticized
and is currently rarely mentioned when discussing the observational properties
of radio pulsars, even though all the criticisms were in their time disproven
in a most thorough and detailed manner. Recent results show even more
conclusively that the theory has no internal inconsistencies. New observational
data also demonstrate the validity of the basic conclusions of the theory.
Based on the latest results on the effects of wave propagation in the
magnetosphere of a neuron star, we show that the developed theory does indeed
allow quantitative predictions of the evolution of neutron stars and the
properties of the observed radio emission.
