Parity nonconservation due to the nuclear weak charge is considered. We demonstrate that the radiative corrections to this effect due to the vacuum fluctuations of the characteristic size larger than the nuclear radius r0 and smaller than the electron Compton wave-length λC are enhanced because of the strong electric field of the nucleus. The parameter that allows one to classify the corrections is the large logarithm ln(λC/r0). The vacuum polarization contribution is enhanced by the second power of the logarithm. Although the self-energy and the vertex corrections do not vanish, they contain only the first power of the logarithm. The value of the radiative correction is 0.4% for Cs and 0.9% for Tl, Pb, and Bi. We discuss also how the correction affects the interpretation of the experimental data on parity nonconservation in atoms. [7,8]. Both the experimental and the theoretical accuracy is best for Cs. Therefore, this atom provides the most important information on the Standard model in the low energy sector. The analysis performed in Ref.[4] has indicated a deviation of the measured weak charge value from that predicted by the Standard model by 2.5 standard deviations σ.In the many-body calculations [6][7][8] the Coulomb interaction between electrons was taken into account, while the magnetic interaction was neglected. The contribution of the magnetic (Breit) electron-electron interaction was calculated in the recent papers [9,10]. It proved to be much larger than a naive estimate, and it shifted the theoretical prediction for PNC in Cs. As a result, the deviation from the Standard model has been reduced. The calculations [9,10] have already been used to get new restrictions on possible modifications of the Standard model, see, e. g., Ref. [11]. The reason for the enhancement of the Breit correction has been explained in Ref. [12]. In the case of the Coulomb residual interaction the effect of the many-body polarization is maximum for the outer electronic subshell and quickly drops down inside the atom [6][7][8]. The Breit interaction is more singular at small distances than the Coulomb one. Hence, the polarization is maximum for the lowest subshell (1s 2 ) and quickly drops down towards the outer shells. The estimate of the relative effect of the magnetic polarization gives Zα 2 instead of naive α 2 , where Z is the nuclear charge and α is the fine structure constant. To find the Breit correction there is no need to repeat the involved many-body calculations performed in Refs. [6][7][8]. Indeed, the Breit correction comes from small distances, r ∼ a B /Z (a B is the Bohr radius), while all the Coulomb polarization and correlation corrections come from large distances, r ∼ a B . Therefore, it is sufficient to calculate the relative Breit correction to some PNC mixing matrix element (say 6s 1/2 − 6p 1/2 mixing in Cs) in the simplest Hartree-Fock or RPA approximation. The relative Breit correction to the PNC effect with account of all manybody Coulomb polarization and correlation corrections is exactly the same...