Atmospheric electric field effect in different neutron multiplicities according to Emilio Segre Obervatory one minute data

On the basis of cosmic ray and atmospherice lectric field one minute data obtained by NM and EFS ofE milio Segre' Observatory (hight 2025 m above s.l., cut-offr igidity for vertical direction 10.8 GV) we determine thea tmospheric electric field effect in CR for total neutroni ntensity and for multiplicities m ≥1, m ≥2, m ≥3, m ≥4,m ≥5, m ≥6, m ≥7, and m ≥8, as well as for m=1, m=2,m =3, m=4, m=5, m=6, and m=7. For comparison ande xcluding primary CR variations we use also data obtainedb y NM of University "Roma Tre" (about sea level, cut-off rigidity 6.7 GV). According to the theoretical calculations of Dorman and Dorman (1995) the electric field effect in the NM counting rate must be caused mainly by catching ofs low negative muons by lead nucleus with escaping fewn eutrons. As it was shown in Dorman et al. (1999), theb iggest electric field effect is expected in the multiplicitym =1, much smaller in m=2 and negligible effect is expected in higher multiplicities. We will control this conclusion ont he basis of our experimental data. Obtained results give a possibility to estimate total acceleration and deceleration of CR particles by the atmospheric electric field._