Filtros : " IFSC224" "Physical Review D" Removidos: "FÍSICA (ENSINO)" "Dobrigkeit, C." "1977" "Neurocomputing" "IF" "IPEN" Limpar

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  • Source: Physical Review D. Unidade: IFSC

    Subjects: RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      LANG, Rodrigo Guedes e TAYLOR, Andrew M. e SOUZA, Vitor de. Ultrahigh-energy cosmic rays dipole and beyond. Physical Review D, v. 103, n. 6, p. 063005-1-063005-12, 2021Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.103.063005. Acesso em: 12 jul. 2024.
    • APA

      Lang, R. G., Taylor, A. M., & Souza, V. de. (2021). Ultrahigh-energy cosmic rays dipole and beyond. Physical Review D, 103( 6), 063005-1-063005-12. doi:10.1103/PhysRevD.103.063005
    • NLM

      Lang RG, Taylor AM, Souza V de. Ultrahigh-energy cosmic rays dipole and beyond [Internet]. Physical Review D. 2021 ; 103( 6): 063005-1-063005-12.[citado 2024 jul. 12 ] Available from: https://doi.org/10.1103/PhysRevD.103.063005
    • Vancouver

      Lang RG, Taylor AM, Souza V de. Ultrahigh-energy cosmic rays dipole and beyond [Internet]. Physical Review D. 2021 ; 103( 6): 063005-1-063005-12.[citado 2024 jul. 12 ] Available from: https://doi.org/10.1103/PhysRevD.103.063005
  • Source: Physical Review D. Unidade: IFSC

    Subjects: FÍSICA DE PARTÍCULAS, RAIOS CÓSMICOS

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      LANG, Rodrigo Guedes et al. Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields. Physical Review D, v. 102, n. 6, p. 063012-01-063012-11, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.102.063012. Acesso em: 12 jul. 2024.
    • APA

      Lang, R. G., Taylor, A. M., Ahlers, M., & Souza, V. de. (2020). Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields. Physical Review D, 102( 6), 063012-01-063012-11. doi:10.1103/PhysRevD.102.063012
    • NLM

      Lang RG, Taylor AM, Ahlers M, Souza V de. Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields [Internet]. Physical Review D. 2020 ; 102( 6): 063012-01-063012-11.[citado 2024 jul. 12 ] Available from: https://doi.org/10.1103/PhysRevD.102.063012
    • Vancouver

      Lang RG, Taylor AM, Ahlers M, Souza V de. Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields [Internet]. Physical Review D. 2020 ; 102( 6): 063012-01-063012-11.[citado 2024 jul. 12 ] Available from: https://doi.org/10.1103/PhysRevD.102.063012
  • Source: Physical Review D. Unidade: IFSC

    Subjects: ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
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    • ABNT

      GENOLINI, Y. et al. Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation. Physical Review D, v. 99, n. 12, p. 123028-1-123028-16, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.99.123028. Acesso em: 12 jul. 2024.
    • APA

      Genolini, Y., Boudaud, M., Batista, P. -I., Caroff, S., Derome, L., Lavalle, J., et al. (2019). Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation. Physical Review D, 99( 12), 123028-1-123028-16. doi:10.1103/PhysRevD.99.123028
    • NLM

      Genolini Y, Boudaud M, Batista P-I, Caroff S, Derome L, Lavalle J, Marcowith A, Maurin D, Poireau V, Poulin V, Rosier S, Salati P, Serpico PD, Vecchi M. Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation [Internet]. Physical Review D. 2019 ; 99( 12): 123028-1-123028-16.[citado 2024 jul. 12 ] Available from: https://doi.org/10.1103/PhysRevD.99.123028
    • Vancouver

      Genolini Y, Boudaud M, Batista P-I, Caroff S, Derome L, Lavalle J, Marcowith A, Maurin D, Poireau V, Poulin V, Rosier S, Salati P, Serpico PD, Vecchi M. Cosmic-ray transport from AMS-02 boron to carbon ratio data: benchmark models and interpretation [Internet]. Physical Review D. 2019 ; 99( 12): 123028-1-123028-16.[citado 2024 jul. 12 ] Available from: https://doi.org/10.1103/PhysRevD.99.123028

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