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This thesis presents an analysis of the cosmic-ray electron and positron fluxusing the AMS-02 detector on the International Space Station as a function oftime and energy. The time-averaged flux is integrated over 6.5 years of AMS-02science data and provides the electron and positron flux with unprecedentedaccuracy, covering the energy range from 0.5 GeV to 1 TeV. In total 28.39million events were identified as electrons and 1.95 million as positrons. Foreach of the 88 Bartels rotation periods (27 days), within the 6.5 years, anindividual electron and positron flux is derived spanning the energy range from1 - 50 GeV.

Precision measurement of the cosmic-ray electron and positron fluxes as  a function of time and energy with the Alpha Magnetic Spectrometer on the  International Space Station