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Spectra of Electrons and Positrons with Energies above 50 MeV, According to Data from the PAMELA Experiment

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

The PAMELA magnetic spectrometer on board the Resurs-DK1 satellite was launched into an elliptical quasipolar Earth orbit with altitudes of 350–600 km and an inclination of ~70° to study the fluxes of cosmic ray particles and antiparticles in a wide range of energies (~50 MeV to hundreds of GeV). Results are presented from observing electron and positron fluxes at energies above 50 MeV between 2006 and 2016.

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Funding

This work was supported by the Russian Foundation for Basic Research, project no. 18-02-00656.

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Authors and Affiliations

  1. National Research Nuclear University, Moscow Engineering Physics Institute (MEPhI), 115409, Moscow, Russia

    V. V. Mikhailov & S. A. Voronov

Authors
  1. V. V. Mikhailov
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  2. S. A. Voronov
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Consortia

on behalf of the PAMELA Collaboration

Corresponding author

Correspondence to V. V. Mikhailov.

Additional information

Translated by E. Smirnova

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Mikhailov, V.V., Voronov, S.A. & on behalf of the PAMELA Collaboration. Spectra of Electrons and Positrons with Energies above 50 MeV, According to Data from the PAMELA Experiment. Bull. Russ. Acad. Sci. Phys. 85, 1036–1038 (2021). https://doi.org/10.3103/S1062873821090239

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  • DOI: https://doi.org/10.3103/S1062873821090239

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