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Observation of Complex Time Structures in the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer on the International Space Station

  • (AMS Collaboration)
  • CIEMAT
  • RWTH Aachen University
  • National Institute for Nuclear Physics
  • Laboratório de Instrumentação e Física Experimental de Partículas
  • Jülich Research Centre
  • Université Grenoble Alpes
  • University of Geneva
  • CERN
  • University of Trento
  • CAS - Institute of High Energy Physics
  • University of Turku
  • ASI
  • Massachusetts Institute of Technology
  • University of Perugia
  • Karlsruhe Institute of Technology
  • University of Hawai'i at Mānoa
  • NASA Johnson Space Center
  • University of Rome La Sapienza
  • Universidade de São Paulo
  • Université Savoie Mont Blanc
  • National Research Council of Italy
  • Ewha Womans University
  • National Central University
  • University of Chinese Academy of Sciences
  • Shandong University

科研成果: 期刊稿件文章同行评审

111 引用 (Scopus)

摘要

We present high-statistics, precision measurements of the detailed time and energy dependence of the primary cosmic-ray electron flux and positron flux over 79 Bartels rotations from May 2011 to May 2017 in the energy range from 1 to 50 GeV. For the first time, the charge-sign dependent modulation during solar maximum has been investigated in detail by leptons alone. Based on 23.5×106 events, we report the observation of short-term structures on the timescale of months coincident in both the electron flux and the positron flux. These structures are not visible in the e+/e- flux ratio. The precision measurements across the solar polarity reversal show that the ratio exhibits a smooth transition over 830±30 days from one value to another. The midpoint of the transition shows an energy dependent delay relative to the reversal and changes by 260±30 days from 1 to 6 GeV.

源语言英语
文章编号051102
期刊Physical Review Letters
121
5
DOI
出版状态已出版 - 31 7月 2018

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