Muons in air showers at the Pierre Auger Observatory: mean number in highly inclined events (2015)
- Authors:
- USP affiliated authors: ALBUQUERQUE, IVONE FREIRE DA MOTA E - IF ; SOUZA FILHO, LUIZ VITOR DE - IFSC ; GOUFFON, PHILIPPE - IF ; SANTOS, EDIVALDO MOURA - IF ; PEIXOTO, CARLOS JOSÉ TODERO - EEL
- Unidades: IF; IFSC; EEL
- DOI: 10.1103/PhysRevD.91.032003
- Subjects: ENERGIA; RAIOS CÓSMICOS; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Publisher place: College Park
- Date published: 2015
- Source:
- Título: Physical Review D
- ISSN: 1550-7998
- Volume/Número/Paginação/Ano: v. 91, n. 3, p. 032003-1-032003-12, Feb. 2015
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
AAB, A. et al. Muons in air showers at the Pierre Auger Observatory: mean number in highly inclined events. Physical Review D, v. 91, n. 3, p. 032003-1-032003-12, 2015Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.91.032003. Acesso em: 24 jan. 2026. -
APA
Aab, A., Albuquerque, I. F. da M. e, Souza, V. de, Gouffon, P., Prado, R. R., Santos, E. M., & Peixoto, C. J. T. (2015). Muons in air showers at the Pierre Auger Observatory: mean number in highly inclined events. Physical Review D, 91( 3), 032003-1-032003-12. doi:10.1103/PhysRevD.91.032003 -
NLM
Aab A, Albuquerque IF da M e, Souza V de, Gouffon P, Prado RR, Santos EM, Peixoto CJT. Muons in air showers at the Pierre Auger Observatory: mean number in highly inclined events [Internet]. Physical Review D. 2015 ; 91( 3): 032003-1-032003-12.[citado 2026 jan. 24 ] Available from: https://doi.org/10.1103/PhysRevD.91.032003 -
Vancouver
Aab A, Albuquerque IF da M e, Souza V de, Gouffon P, Prado RR, Santos EM, Peixoto CJT. Muons in air showers at the Pierre Auger Observatory: mean number in highly inclined events [Internet]. Physical Review D. 2015 ; 91( 3): 032003-1-032003-12.[citado 2026 jan. 24 ] Available from: https://doi.org/10.1103/PhysRevD.91.032003 - A targeted search for point sources of EeV neutrons
- Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
- Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger Observatory with Zenith angles up to 80°
- Nanosecond-level time synchronization of autonomous radio detector stations for extensive air showers
- Prototype muon detectors for the AMIGA component of the Pierre Auger Observatory
- Search for correlations between the arrival directions of IceCube neutrino events and ultrahigh-energy cosmic rays detected by the Pierre Auger Observatory and the Telescope Array
- Searches for large-scale anisotropy in the arrival directions of cosmic rays detected above energy of '10 POT. 19' eV at the Pierre Auger observatory and the telescope array
- Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory
- Search for ultrarelativistic magnetic monopoles with the Pierre Auger observatory
- Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy
Informações sobre o DOI: 10.1103/PhysRevD.91.032003 (Fonte: oaDOI API)
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