  During the last few years there were discovered and deeply examined several
transient neutron stars (Rotating Radio Transients). It is already well
accepted that these objects are rotating neutron stars. But their extraordinary
features (burst-like behavior) made necessary revision of well accepted models
of pulsar interior structure. Nowadays most popular model for RRATs is
precessing pulsar model, which is the subject of big discussion. We assume that
these objects are pulsars with specific spin parameters. An important feature
of our model, naturally explaining most of the properties of these neutron
stars, is presence of very low frequency, nearly transverse drift waves
propagating across the magnetic field and encircling the open field lines
region of the pulsar magnetosphere.
