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Here we discuss a method for a study of the heavy nuclei cosmic ray composition. The method is based on a charge separation with the PAMELA calorimeter. The work is in progress now. The ability is presented to carry out measurements up to Fe and Ni. As a result we expect to get important data about the abundance of the chemical elements in the cosmic rays.doi:10.1088/1742-6596/678/1/012062 fatcat:lbctb3kix5dxlnfabd5hc34m7u