As galactic cosmic rays (GCRs) diffuse into the heliosphere, their energy spectra are distorted by interactions with the magnetic field convected outward by the expanding solar wind. This process, called solar modulation, will cause GCRs with interstellar energies less than ~1 GeV/nucleon to lose a significant fraction of their energy due to adiabatic deceleration; these losses are smallest during the solar minimum periods of the ~11 year solar cycle.