Self-Action Effects In the Theory of Classical Spinning Charge

The back-reaction effects for the spinning charge moving through the constant homogeneous electromagnetic field are studied in the context of the mass-shift (MS) method. For the g=2 magnetic moment case we find the (complex) addition to the classical action. Its dependence on the integrals of the unperturbed motion proves to be important in determination of the orbital radiation effects and could assist in understanding the radiation polarization (RP) phenomenon.