Filtros : "Bueno, E. F." "Physical Review Letters" "IFSC" Removido: "Universidade Estadual de Campinas (UNICAMP)" Limpar

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  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Towards understanding the origin of cosmic-ray positrons. Physical Review Letters, v. 122, n. 4, p. 041102-1-041102-9, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.122.041102. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., & Vecchi, M. (2019). Towards understanding the origin of cosmic-ray positrons. Physical Review Letters, 122( 4), 041102-1-041102-9. doi:10.1103/PhysRevLett.122.041102
    • NLM

      Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray positrons [Internet]. Physical Review Letters. 2019 ; 122( 4): 041102-1-041102-9.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.122.041102
    • Vancouver

      Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray positrons [Internet]. Physical Review Letters. 2019 ; 122( 4): 041102-1-041102-9.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.122.041102
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Towards understanding the origin of cosmic-ray electrons. Physical Review Letters, v. 122, n. 10, p. 101101-1-101101-9, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.122.101101. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., & Vecchi, M. (2019). Towards understanding the origin of cosmic-ray electrons. Physical Review Letters, 122( 10), 101101-1-101101-9. doi:10.1103/PhysRevLett.122.101101
    • NLM

      Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray electrons [Internet]. Physical Review Letters. 2019 ; 122( 10): 101101-1-101101-9.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.122.101101
    • Vancouver

      Aguilar M, Bueno EF, Vecchi M. Towards understanding the origin of cosmic-ray electrons [Internet]. Physical Review Letters. 2019 ; 122( 10): 101101-1-101101-9.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.122.101101
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. et al. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051101-1-051101-7, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051101. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051101-1-051101-7. doi:10.1103/PhysRevLett.121.051101
    • NLM

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051101-1-051101-7.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051101
    • Vancouver

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051101-1-051101-7.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051101
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. et al. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051102-1-051102-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051102. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051102-1-051102-8. doi:10.1103/PhysRevLett.121.051102
    • NLM

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051102-1-051102-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051102
    • Vancouver

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051102-1-051102-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051102
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. et al. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 120, n. Ja 2018, p. 021101-1-021101-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.120.021101. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station. Physical Review Letters, 120( Ja 2018), 021101-1-021101-8. doi:10.1103/PhysRevLett.120.021101
    • NLM

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 120( Ja 2018): 021101-1-021101-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.120.021101
    • Vancouver

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 120( Ja 2018): 021101-1-021101-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.120.021101
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. et al. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 121, n. 5, p. 051103-1-051103-8, 2018Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.121.051103. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2018). Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 121( 5), 051103-1-051103-8. doi:10.1103/PhysRevLett.121.051103
    • NLM

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051103-1-051103-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051103
    • Vancouver

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of cosmic-ray nitrogen and its primary and secondary components with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2018 ; 121( 5): 051103-1-051103-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.121.051103
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. et al. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 119, n. 25, p. 251101-1-241101-8, 2017Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.119.251101. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2017). Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station. Physical Review Letters, 119( 25), 251101-1-241101-8. doi:10.1103/PhysRevLett.119.251101
    • NLM

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2017 ; 119( 25): 251101-1-241101-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.119.251101
    • Vancouver

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2017 ; 119( 25): 251101-1-241101-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.119.251101
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Acesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. e BUENO, E. F. e VECCHI, Manuela. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station. Physical Review Letters, v. 117, n. 9, p. 091103-1-091103-10, 2016Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.117.091103. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., & Vecchi, M. (2016). Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station. Physical Review Letters, 117( 9), 091103-1-091103-10. doi:10.1103/PhysRevLett.117.091103
    • NLM

      Aguilar M, Bueno EF, Vecchi M. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station [Internet]. Physical Review Letters. 2016 ; 117( 9): 091103-1-091103-10.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.117.091103
    • Vancouver

      Aguilar M, Bueno EF, Vecchi M. Antiproton flux, antiproton-to-proton flux ratio, and properties of elementary particle fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the International Space Station [Internet]. Physical Review Letters. 2016 ; 117( 9): 091103-1-091103-10.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.117.091103
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Acesso à fonteDOIHow to cite
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    • ABNT

      AGUILAR, M. et al. Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. 117, n. 23, p. 231102-1-231102-8, 2016Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.117.231102. Acesso em: 17 jun. 2024.
    • APA

      Aguilar, M., Bueno, E. F., Lordello, V. D., Mikuni, V. M., & Vecchi, M. (2016). Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station. Physical Review Letters, 117( 23), 231102-1-231102-8. doi:10.1103/PhysRevLett.117.231102
    • NLM

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2016 ; 117( 23): 231102-1-231102-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.117.231102
    • Vancouver

      Aguilar M, Bueno EF, Lordello VD, Mikuni VM, Vecchi M. Precision measurement of the boron to carbon flux ratio in cosmic rays from 1.9 GV to 2.6 TV with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2016 ; 117( 23): 231102-1-231102-8.[citado 2024 jun. 17 ] Available from: https://doi.org/10.1103/PhysRevLett.117.231102

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