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Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components 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
  • Middle East Technical University
  • 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
  • National Research Council of Italy
  • 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

102 引用 (Scopus)

摘要

A precision measurement of the nitrogen flux with rigidity (momentum per unit charge) from 2.2 GV to 3.3 TV based on 2.2×106 events is presented. The detailed rigidity dependence of the nitrogen flux spectral index is presented for the first time. The spectral index rapidly hardens at high rigidities and becomes identical to the spectral indices of primary He, C, and O cosmic rays above ∼700 GV. We observed that the nitrogen flux ΦN can be presented as the sum of its primary component ΦNP and secondary component ΦNS, ΦN=ΦNP+ΦNS, and we found ΦN is well described by the weighted sum of the oxygen flux ΦO (primary cosmic rays) and the boron flux ΦB (secondary cosmic rays), with ΦNP=(0.090±0.002)×ΦO and ΦNS=(0.62±0.02)×ΦB over the entire rigidity range. This corresponds to a change of the contribution of the secondary cosmic ray component in the nitrogen flux from 70% at a few GV to <30% above 1 TV.

源语言英语
文章编号051103
期刊Physical Review Letters
121
5
DOI
出版状态已出版 - 31 7月 2018

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