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Temporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Rays

M. Aguilar et al. (AMS Collaboration)
Phys. Rev. Lett. 130, 161001 – Published 17 April 2023
Physics logo See Viewpoint: Disentangling the Sun’s Impact on Cosmic Rays
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Abstract

We present the precision measurements of 11 years of daily cosmic electron fluxes in the rigidity interval from 1.00 to 41.9 GV based on 2.0×108 electrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The electron fluxes exhibit variations on multiple timescales. Recurrent electron flux variations with periods of 27 days, 13.5 days, and 9 days are observed. We find that the electron fluxes show distinctly different time variations from the proton fluxes. Remarkably, a hysteresis between the electron flux and the proton flux is observed with a significance of greater than 6σ at rigidities below 8.5 GV. Furthermore, significant structures in the electron-proton hysteresis are observed corresponding to sharp structures in both fluxes. This continuous daily electron data provide unique input to the understanding of the charge sign dependence of cosmic rays over an 11-year solar cycle.

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  • Received 22 September 2022
  • Revised 21 November 2022
  • Accepted 9 February 2023

DOI:https://doi.org/10.1103/PhysRevLett.130.161001

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

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Disentangling the Sun’s Impact on Cosmic Rays

Published 17 April 2023

An instrument on the International Space Station has revealed new information about how the Sun’s magnetic field affects cosmic rays on their way to Earth.

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Vol. 130, Iss. 16 — 21 April 2023

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