The PAMELA experiment had operated almost ten years on board of the Resurs DK1 satellite. The satellite was launched on the 15$^{th}$ of June 2006 and placed in orbit with an inclination of 70° and an altitude of 350 to 610 km. The experiment had continuously measured electron and positron fluxes of Galactic cosmic rays in a wide energy range from about 50 MeV to hundreds of GeV. The spectra of electrons %and positrons
have been analysed from the end of 23$^{rd}$ until the beginning of 24$^{th}$ solar cycle including the prolonged deep solar minimum period from 2006 to the end of 2009 and the solar magnetic polarity reversal period in 2012-2014. Here, we present updated annual electron spectra from 2006 to 2015.
Study of the modulation of Galactic positrons and electrons in 2006-2016 with the PAMELA Experiment
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Pre-published on:
July 29, 2021
Published on:
March 18, 2022
Abstract
DOI: https://doi.org/10.22323/1.395.1307
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.