Source: Physical Review D. Unidade: IFSC
Subjects: ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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: 03 set. 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.99.123028NLM
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 set. 03 ] Available from: https://doi.org/10.1103/PhysRevD.99.123028Vancouver
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 set. 03 ] Available from: https://doi.org/10.1103/PhysRevD.99.123028