The parameters of the electron-positron plasma and intensity of X-ray
emission from hot spots in the polar regions of radio pulsars are calc
ulated using a Goldreich-Julian model in the regime of free electron e
mission from the neutron star surface. In this case, the electric fiel
d is generated by the general relativistic effect of inertial frame dr
agging. The results obtained are in agreement with the observational d
ata for the radio pulsars PSR 1055-52 and PSR 1929+10, and for the Gem
inga pulsar (E0630+18).