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  • Source: Physical Review Letters. Unidades: EEL, IFSC, IF

    Subjects: RAIOS CÓSMICOS, FÍSICA DE ALTA ENERGIA, ASTROFÍSICA

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      AAB, A. et al. Measurement of the fluctuations in the number of muons in extensive air Showers with the Pierre Auger Observatory. Physical Review Letters, v. 126, n. 15, p. 152002-1-152002-11, 2021Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.126.152002. Acesso em: 28 out. 2024.
    • APA

      Aab, A., Arbeletche, L. B., Catalani, F., Souza, V. de, Lang, R. G., Martínez-Huerta, H., et al. (2021). Measurement of the fluctuations in the number of muons in extensive air Showers with the Pierre Auger Observatory. Physical Review Letters, 126( 15), 152002-1-152002-11. doi:10.1103/PhysRevLett.126.152002
    • NLM

      Aab A, Arbeletche LB, Catalani F, Souza V de, Lang RG, Martínez-Huerta H, Armand JP, Carvalho Junior WR de, Santos EM, Peixoto CJT. Measurement of the fluctuations in the number of muons in extensive air Showers with the Pierre Auger Observatory [Internet]. Physical Review Letters. 2021 ; 126( 15): 152002-1-152002-11.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.126.152002
    • Vancouver

      Aab A, Arbeletche LB, Catalani F, Souza V de, Lang RG, Martínez-Huerta H, Armand JP, Carvalho Junior WR de, Santos EM, Peixoto CJT. Measurement of the fluctuations in the number of muons in extensive air Showers with the Pierre Auger Observatory [Internet]. Physical Review Letters. 2021 ; 126( 15): 152002-1-152002-11.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.126.152002
  • Source: Physical Review Letters. Unidade: IFSC

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

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      ALBERT, A e MARTÍNEZ-HUERTA, Humberto. Constraints on Lorentz invariance violation from HAWC observations of gamma rays above 100 TeV. Physical Review Letters, v. 124, n. 13, p. 131101-131101-7, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.124.131101. Acesso em: 28 out. 2024.
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      Albert, A., & Martínez-Huerta, H. (2020). Constraints on Lorentz invariance violation from HAWC observations of gamma rays above 100 TeV. Physical Review Letters, 124( 13), 131101-131101-7. doi:10.1103/PhysRevLett.124.131101
    • NLM

      Albert A, Martínez-Huerta H. Constraints on Lorentz invariance violation from HAWC observations of gamma rays above 100 TeV [Internet]. Physical Review Letters. 2020 ; 124( 13): 131101-131101-7.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.124.131101
    • Vancouver

      Albert A, Martínez-Huerta H. Constraints on Lorentz invariance violation from HAWC observations of gamma rays above 100 TeV [Internet]. Physical Review Letters. 2020 ; 124( 13): 131101-131101-7.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.124.131101
  • Source: Physical Review Letters. Unidades: EEL, IFSC, IF

    Subjects: RAIOS CÓSMICOS, FÍSICA DE ALTA ENERGIA, ASTROFÍSICA

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      AAB, A. et al. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory. Physical Review Letters, v. 125, n. 12, p. 121106-1-121106-10, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.125.121106. Acesso em: 28 out. 2024.
    • APA

      Aab, A., Arbeletche, L. B., Catalani, F., Souza, V. de, Lang, R. G., Martínez-Huerta, H., et al. (2020). Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory. Physical Review Letters, 125( 12), 121106-1-121106-10. doi:10.1103/PhysRevLett.125.121106
    • NLM

      Aab A, Arbeletche LB, Catalani F, Souza V de, Lang RG, Martínez-Huerta H, Armand JP, Carvalho Junior WR de, Santos EM, Peixoto CJT. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory [Internet]. Physical Review Letters. 2020 ; 125( 12): 121106-1-121106-10.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.125.121106
    • Vancouver

      Aab A, Arbeletche LB, Catalani F, Souza V de, Lang RG, Martínez-Huerta H, Armand JP, Carvalho Junior WR de, Santos EM, Peixoto CJT. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory [Internet]. Physical Review Letters. 2020 ; 125( 12): 121106-1-121106-10.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.125.121106
  • Source: Physical Review Letters. Unidade: IFSC

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

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      ABEYSEKARA, A. U. e MARTÍNEZ-HUERTA, Humberto. Multiple galactic sources with emission above 56 TeV detected by HAWC. Physical Review Letters, v. 124, n. Ja 2020, p. 021102-1-1-021102-7, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.124.021102. Acesso em: 28 out. 2024.
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      Abeysekara, A. U., & Martínez-Huerta, H. (2020). Multiple galactic sources with emission above 56 TeV detected by HAWC. Physical Review Letters, 124( Ja 2020), 021102-1-1-021102-7. doi:10.1103/PhysRevLett.124.021102
    • NLM

      Abeysekara AU, Martínez-Huerta H. Multiple galactic sources with emission above 56 TeV detected by HAWC [Internet]. Physical Review Letters. 2020 ; 124( Ja 2020): 021102-1-1-021102-7.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.124.021102
    • Vancouver

      Abeysekara AU, Martínez-Huerta H. Multiple galactic sources with emission above 56 TeV detected by HAWC [Internet]. Physical Review Letters. 2020 ; 124( Ja 2020): 021102-1-1-021102-7.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.124.021102
  • Source: Physical Review Letters. Unidade: IFSC

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

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      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: 28 out. 2024.
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      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 out. 28 ] 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 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.122.041102
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: RAIOS CÓSMICOS, ASTROFÍSICA, ISÓTOPOS, ESPECTROMETRIA

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      AGUILAR, M. e VECCHI, Manuela. Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer. Physical Review Letters, v. No 2019, n. 18, p. 181102-1-181102-8, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.123.181102. Acesso em: 28 out. 2024.
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      Aguilar, M., & Vecchi, M. (2019). Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer. Physical Review Letters, No 2019( 18), 181102-1-181102-8. doi:10.1103/PhysRevLett.123.181102
    • NLM

      Aguilar M, Vecchi M. Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer [Internet]. Physical Review Letters. 2019 ; No 2019( 18): 181102-1-181102-8.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.123.181102
    • Vancouver

      Aguilar M, Vecchi M. Properties of cosmic helium isotopes measured by the alpha magnetic spectrometer [Internet]. Physical Review Letters. 2019 ; No 2019( 18): 181102-1-181102-8.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.123.181102
  • Source: Physical Review Letters. Unidade: IFSC

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

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      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: 28 out. 2024.
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      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 out. 28 ] 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 out. 28 ] 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

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      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: 28 out. 2024.
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      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 out. 28 ] 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 out. 28 ] 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

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      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: 28 out. 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 out. 28 ] 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 out. 28 ] 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

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      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: 28 out. 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 out. 28 ] 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 out. 28 ] 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

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      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: 28 out. 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 out. 28 ] 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 out. 28 ] 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

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      GÉNOLINI, Yoann et al. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient. Physical Review Letters, v. 119, n. 24, p. 241101-1-241101-6, 2017Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.119.241101. Acesso em: 28 out. 2024.
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      Génolini, Y., Serpico, P. D., Boudaud, M., Caroff, S., Poulin, V., Derome, L., et al. (2017). Indications for a high-rigidity break in the cosmic-ray diffusion coefficient. Physical Review Letters, 119( 24), 241101-1-241101-6. doi:10.1103/PhysRevLett.119.241101
    • NLM

      Génolini Y, Serpico PD, Boudaud M, Caroff S, Poulin V, Derome L, Lavalle J, Maurin D, Poireau V, Rosier S, Salati P, Vecchi M. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient [Internet]. Physical Review Letters. 2017 ; 119( 24): 241101-1-241101-6.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.119.241101
    • Vancouver

      Génolini Y, Serpico PD, Boudaud M, Caroff S, Poulin V, Derome L, Lavalle J, Maurin D, Poireau V, Rosier S, Salati P, Vecchi M. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient [Internet]. Physical Review Letters. 2017 ; 119( 24): 241101-1-241101-6.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.119.241101
  • Source: Physical Review Letters. Unidade: IFSC

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

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      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: 28 out. 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 out. 28 ] 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 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.119.251101
  • Source: Physical Review Letters. Unidades: IF, IFSC, EEL

    Subjects: ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

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      AAB, A. et al. Testing hadronic interactions at ultrahigh energies with air showers measured by the Pierre Auger Observatory. Physical Review Letters, v. No 2016, n. 19, p. 192001-1-192001-9, 2016Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.117.192001. Acesso em: 28 out. 2024.
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      Aab, A., Albuquerque, I. F. da M. e, Souza, V. de, Gouffon, P., Prado, R. R., Santos, E. M., & Peixoto, C. J. T. (2016). Testing hadronic interactions at ultrahigh energies with air showers measured by the Pierre Auger Observatory. Physical Review Letters, No 2016( 19), 192001-1-192001-9. doi:10.1103/PhysRevLett.117.192001
    • NLM

      Aab A, Albuquerque IF da M e, Souza V de, Gouffon P, Prado RR, Santos EM, Peixoto CJT. Testing hadronic interactions at ultrahigh energies with air showers measured by the Pierre Auger Observatory [Internet]. Physical Review Letters. 2016 ; No 2016( 19): 192001-1-192001-9.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.117.192001
    • Vancouver

      Aab A, Albuquerque IF da M e, Souza V de, Gouffon P, Prado RR, Santos EM, Peixoto CJT. Testing hadronic interactions at ultrahigh energies with air showers measured by the Pierre Auger Observatory [Internet]. Physical Review Letters. 2016 ; No 2016( 19): 192001-1-192001-9.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.117.192001
  • Source: Physical Review Letters. Unidade: IFSC

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

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      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: 28 out. 2024.
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      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 out. 28 ] 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 out. 28 ] 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

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      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: 28 out. 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 out. 28 ] 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 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.117.231102
  • Source: Physical Review Letters. Unidades: IF, IFSC, EEL

    Subjects: ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      AAB, A. et al. Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy. Physical Review Letters, v. No 2016, n. 24, p. 211101-1-211101-9, 2016Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.116.241101. Acesso em: 28 out. 2024.
    • APA

      Aab, A., Albuquerque, I. F. da M. e, Souza, V. de, Anjos, R. C., Gouffon, P., Prado, R. R., et al. (2016). Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy. Physical Review Letters, No 2016( 24), 211101-1-211101-9. doi:10.1103/PhysRevLett.116.241101
    • NLM

      Aab A, Albuquerque IF da M e, Souza V de, Anjos RC, Gouffon P, Prado RR, Santos EM, Peixoto CJT. Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy [Internet]. Physical Review Letters. 2016 ; No 2016( 24): 211101-1-211101-9.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.116.241101
    • Vancouver

      Aab A, Albuquerque IF da M e, Souza V de, Anjos RC, Gouffon P, Prado RR, Santos EM, Peixoto CJT. Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy [Internet]. Physical Review Letters. 2016 ; No 2016( 24): 211101-1-211101-9.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.116.241101
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

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    • ABNT

      AGUILAR, M. e VECCHI, Manuela. Precision measurement of the helium flux in primary cosmic rays of rigidities 1.9 GV to 3 TV with the alpha magnetic spectrometer on the international space station. Physical Review Letters, v. No 2015, n. 21, p. 211101-1-211101-9, 2015Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.115.211101. Acesso em: 28 out. 2024.
    • APA

      Aguilar, M., & Vecchi, M. (2015). Precision measurement of the helium flux in primary cosmic rays of rigidities 1.9 GV to 3 TV with the alpha magnetic spectrometer on the international space station. Physical Review Letters, No 2015( 21), 211101-1-211101-9. doi:10.1103/PhysRevLett.115.211101
    • NLM

      Aguilar M, Vecchi M. Precision measurement of the helium flux in primary cosmic rays of rigidities 1.9 GV to 3 TV with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2015 ; No 2015( 21): 211101-1-211101-9.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.115.211101
    • Vancouver

      Aguilar M, Vecchi M. Precision measurement of the helium flux in primary cosmic rays of rigidities 1.9 GV to 3 TV with the alpha magnetic spectrometer on the international space station [Internet]. Physical Review Letters. 2015 ; No 2015( 21): 211101-1-211101-9.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.115.211101
  • Source: Physical Review Letters. Unidades: IFSC, IF

    Subjects: ASTROFÍSICA, FÍSICA DE PARTÍCULAS, RAIOS CÓSMICOS, NEUTRINOS, TELESCÓPIOS

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    • ABNT

      ABREU, P. et al. Measurement of the proton-air cross section at 's POT. 1/2' = 57 TeV with the Pierre Auger Observatory. Physical Review Letters, v. 109, n. 6, p. 062002-1-062002-9, 2012Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.109.062002. Acesso em: 28 out. 2024.
    • APA

      Abreu, P., Albuquerque, I. F. M., Souza, V. de, Gouffon, P., Carvalho, W. R. de, Peixoto, C. J. T., & Tridapalli, D. B. (2012). Measurement of the proton-air cross section at 's POT. 1/2' = 57 TeV with the Pierre Auger Observatory. Physical Review Letters, 109( 6), 062002-1-062002-9. doi:10.1103/PhysRevLett.109.062002
    • NLM

      Abreu P, Albuquerque IFM, Souza V de, Gouffon P, Carvalho WR de, Peixoto CJT, Tridapalli DB. Measurement of the proton-air cross section at 's POT. 1/2' = 57 TeV with the Pierre Auger Observatory [Internet]. Physical Review Letters. 2012 ; 109( 6): 062002-1-062002-9.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.109.062002
    • Vancouver

      Abreu P, Albuquerque IFM, Souza V de, Gouffon P, Carvalho WR de, Peixoto CJT, Tridapalli DB. Measurement of the proton-air cross section at 's POT. 1/2' = 57 TeV with the Pierre Auger Observatory [Internet]. Physical Review Letters. 2012 ; 109( 6): 062002-1-062002-9.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.109.062002
  • Source: Physical Review Letters. Unidade: IFSC

    Subjects: RAIOS CÓSMICOS, ESPECTROS, ENERGIA

    Acesso à fonteDOIHow to cite
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    • ABNT

      APEL, W. D. et al. Kneelike structure in the spectrum of the heavy component of cosmic rays observed with KASCADE-Grande. Physical Review Letters, v. 107, n. 17, p. 171104-1-171104-5, 2011Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.107.171104. Acesso em: 28 out. 2024.
    • APA

      Apel, W. D., Arteaga-Velazquez, J. C., Bekk, K., Bertaina, M., Blümer, J., Bozdog, H., et al. (2011). Kneelike structure in the spectrum of the heavy component of cosmic rays observed with KASCADE-Grande. Physical Review Letters, 107( 17), 171104-1-171104-5. doi:10.1103/PhysRevLett.107.171104
    • NLM

      Apel WD, Arteaga-Velazquez JC, Bekk K, Bertaina M, Blümer J, Bozdog H, Brancus IM, Buchholz P, Cantoni E, Chiavassa A, Cossavella F, Daumiller K, Souza V de, Di Pierro F, Doll P, Engel R, Engler J, Finger M, Fuhrmann D, Ghia PL, Gils HJ, Glasstetter R, Grupen C, Haungs A, Heck D, Hörandel JR, Huber D, Huege T, Isar PG, Kampert K-H, Kang D, Klages HO, Link K, Luczak P, Ludwig M, Mathes HJ, Mayer HJ, Melissas M, Milke J, Mitrica B, Morello C, Navarra G, Oehlschläeger J, Ostapchenko S, Over S, Palmieri N, Petcu M, Pierog T, Rebel H, Roth M, Schieler H, Schröder FG, Sima O, Toma G, Trinchero GC, Ulrich H, Weindl A, Wochele J, Wommer M, Zabierowski J. Kneelike structure in the spectrum of the heavy component of cosmic rays observed with KASCADE-Grande [Internet]. Physical Review Letters. 2011 ; 107( 17): 171104-1-171104-5.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.107.171104
    • Vancouver

      Apel WD, Arteaga-Velazquez JC, Bekk K, Bertaina M, Blümer J, Bozdog H, Brancus IM, Buchholz P, Cantoni E, Chiavassa A, Cossavella F, Daumiller K, Souza V de, Di Pierro F, Doll P, Engel R, Engler J, Finger M, Fuhrmann D, Ghia PL, Gils HJ, Glasstetter R, Grupen C, Haungs A, Heck D, Hörandel JR, Huber D, Huege T, Isar PG, Kampert K-H, Kang D, Klages HO, Link K, Luczak P, Ludwig M, Mathes HJ, Mayer HJ, Melissas M, Milke J, Mitrica B, Morello C, Navarra G, Oehlschläeger J, Ostapchenko S, Over S, Palmieri N, Petcu M, Pierog T, Rebel H, Roth M, Schieler H, Schröder FG, Sima O, Toma G, Trinchero GC, Ulrich H, Weindl A, Wochele J, Wommer M, Zabierowski J. Kneelike structure in the spectrum of the heavy component of cosmic rays observed with KASCADE-Grande [Internet]. Physical Review Letters. 2011 ; 107( 17): 171104-1-171104-5.[citado 2024 out. 28 ] Available from: https://doi.org/10.1103/PhysRevLett.107.171104

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