Abstract
An analysis of long-term observations of the fluxes of interplanetary protons with energies of 1–100 MeV measured at a distance of 1 AU from the Sun is performed. The results from computations of the maximum, average, and minimum values of total interplanetary proton fluences accumulated over periods ranging from 1 month to 10 years are presented. The possibilities of applying the obtained data to characterizing and predicting space weather and climate are discussed.
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