Аннотация:Analysis of long-term observations of the fluxes of interplanetary protons with energies from 1 to >100 MeV measured at a distance of 1 AU from the Sun has been carried out. The results of computations of the maximal, mean and minimal values of total interplanetary proton fluences accumulated over the periods from 3
months to 10 years are presented. Possibilities of application of the obtained data for the characterization and prediction of solar weather and climate are discussed.