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1978), A technique to determine the charge state of anomalous low-energy cosmic rays, in 15th International Cos-(1996), New high temporal and spatial resolution measurements by SAMPEX of the precipitation of relativistic electrons,

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Gamma ray line emission from nuclear deexcitation following ener getic particle reactions is evaluated. The compiled nuclear data and the calculated gamma ray spectra and intensities can be used for the study of astrophysical sites which contain large fluxes of energetic protons and nuclei. A detailed evaluation of gamma ray line production in the interstellar medium is made in the present paper.