Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum (2016)
- Authors:
- USP affiliated authors: ALBUQUERQUE, IVONE FREIRE DA MOTA E - IF ; SOUZA FILHO, LUIZ VITOR DE - IFSC ; GOUFFON, PHILIPPE - IF ; PEIXOTO, CARLOS JOSÉ TODERO - EEL
- Unidades: IF; IFSC; EEL
- DOI: 10.1016/j.physletb.2016.09.039
- Subjects: RAIOS CÓSMICOS; ASTROFÍSICA; OBSERVATÓRIOS
- Keywords: Pierre Auger Observatory; Cosmic rays; Mass composition; Ankle
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Physics Letters B
- ISSN: 0370-2693
- Volume/Número/Paginação/Ano: v. 762, p. 288-295, Nov. 2016
- Este periódico é de acesso aberto
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: gold
- Licença: cc-by
-
ABNT
AAB, A. et al. Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum. Physics Letters B, v. No 2016, p. 288-295, 2016Tradução . . Disponível em: https://doi.org/10.1016/j.physletb.2016.09.039. Acesso em: 18 set. 2024. -
APA
Aab, A., Albuquerque, I. F. da M. e, Souza, V. de, Gouffon, P., Prado, R. R., & Peixoto, C. J. T. (2016). Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum. Physics Letters B, No 2016, 288-295. doi:10.1016/j.physletb.2016.09.039 -
NLM
Aab A, Albuquerque IF da M e, Souza V de, Gouffon P, Prado RR, Peixoto CJT. Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum [Internet]. Physics Letters B. 2016 ; No 2016 288-295.[citado 2024 set. 18 ] Available from: https://doi.org/10.1016/j.physletb.2016.09.039 -
Vancouver
Aab A, Albuquerque IF da M e, Souza V de, Gouffon P, Prado RR, Peixoto CJT. Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum [Internet]. Physics Letters B. 2016 ; No 2016 288-295.[citado 2024 set. 18 ] Available from: https://doi.org/10.1016/j.physletb.2016.09.039 - Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America
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Informações sobre o DOI: 10.1016/j.physletb.2016.09.039 (Fonte: oaDOI API)
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