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Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
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Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
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Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment

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Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
Journal Article

Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment

2019
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Overview
AbstractThe PAMELA magnetic spectrometer was launched onboard the Resurs-DK1 satellite into a near-polar Earth orbit with an altitude of 350–600 km, in order to study fluxes of cosmic ray particles and antiparticles in the wide energy range of ~80 MeV to hundreds of GeV. The results from observations of electron and positron fluxes in 2006–2016 are presented.

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