Abstract
The results from measurements of the isotopic composition of nuclei from hydrogen to beryllium in galactic cosmic rays observed in the orbital experiment near the solar activity minimum in 2006–2008 by analyzing the loss of nucleus ionization with the rigidity known from measuring the trajectories for particles passed through the device without nuclear interaction in the multilayer calorimeter of the PAMELA magnetic spectrometer are presented. The results from measurements are compared to existing experimental and calculated data.
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