From the moment of their formation all particles produced by a primary cosmic ray are influenced by atmospheric conditions, such as pressure, temperature, air density, and others. Atmospheric Electric Field (AEF) is one of these factors. There is evidence of a considerable increase of the counting rate of particles during electrical storms. In the present work at the Chacaltaya Cosmic Rays Physics Laboratory (5220 m a.s.l.), the existent relation between AEF and secondary particles produced by primary cosmic rays under two different weather conditions is searched, during fair weather days and disturbed weather days.