Propagation of Cosmic Ray Electron Component in the Galaxy

Physics

Scientific paper

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Scientific paper

A detailed calculation has been carried out to determine the energy spectrum of positrons in the Galaxy. These calculations are compared with the observed spectrum and useful information on the magnitude of modulation is obtained. In the case of electrons, a source spectrum has been added and constraints has been set on the spectrum. It is shown that the charge-sign effect on solar modulation is required. Finally, a consistency check has been made by comparing the estimated fraction of positrons with the observed data.

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