Precision measurements of the electron component in the cosmic radiation provide important information about the origin and propagation of cosmic rays in the Galaxy. Here we present new results regarding negatively charged electrons between 1 and 625 GeV performed by the satellite-borne experiment PAMELA. This is the first time that cosmic-ray e

Cosmic-Ray Electron Flux Measured by the PAMELA Experiment between 1 and 625 GeV

BELLOTTI, Roberto;
2011-01-01

Abstract

Precision measurements of the electron component in the cosmic radiation provide important information about the origin and propagation of cosmic rays in the Galaxy. Here we present new results regarding negatively charged electrons between 1 and 625 GeV performed by the satellite-borne experiment PAMELA. This is the first time that cosmic-ray e
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11586/86451
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