The effect of cosmic ray energy changes in the heliosphere on K-capture

In an accompanying paper we give a re-assessment of cosmic ray energy changes in the heliosphere to determine the effects of acceleration at the solar wind termination shock and modulation in the heliosheath beyond that. In this paper we show that these effects have important consequences for the interpretation of secondary to primary ratios of cosmic rays at energies below 1 GeV, i.e. in the region where they are strongly modulated