The production of electron-positron bunches in a pulsar magnetosphere and their thermal radioemission

It is shown that the high brightness temperature of pulsar radioemission, its sharp directivity and some general features of pulsar radiospectra can be obtained as a corollary of the general statistical regularities of motion of electron-positron bunches in a strong magnetic field. The production mechanism of the bunches is considered and their energy and sizes are estimated. In the presented pulsar model, the energy of accelerated electrons is estimated.