Cosmic rays: the spectrum and chemical composition from '10 POT. 10' to '10 POT. 20' eV (2015)
- Authors:
- USP affiliated authors: PEIXOTO, CARLOS JOSÉ TODERO - EEL ; SOUZA FILHO, LUIZ VITOR DE - IFSC
- Unidades: EEL; IFSC
- DOI: 10.1088/1475-7516/2015/07/042
- Subjects: FÍSICA DE ALTA ENERGIA; RAIOS CÓSMICOS; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Source:
- Título: Journal of Cosmology and Astroparticle Physics
- ISSN: 1475-7516
- Volume/Número/Paginação/Ano: v. 2015, p. 42-1-42-12, July 2015
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
ABNT
PEIXOTO, Carlos Jose Todero e SOUZA, Vitor de e BIERMANN, Peter L. Cosmic rays: the spectrum and chemical composition from '10 POT. 10' to '10 POT. 20' eV. Journal of Cosmology and Astroparticle Physics, v. 2015, p. 42-1-42-12, 2015Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2015/07/042. Acesso em: 26 dez. 2025. -
APA
Peixoto, C. J. T., Souza, V. de, & Biermann, P. L. (2015). Cosmic rays: the spectrum and chemical composition from '10 POT. 10' to '10 POT. 20' eV. Journal of Cosmology and Astroparticle Physics, 2015, 42-1-42-12. doi:10.1088/1475-7516/2015/07/042 -
NLM
Peixoto CJT, Souza V de, Biermann PL. Cosmic rays: the spectrum and chemical composition from '10 POT. 10' to '10 POT. 20' eV [Internet]. Journal of Cosmology and Astroparticle Physics. 2015 ; 2015 42-1-42-12.[citado 2025 dez. 26 ] Available from: https://doi.org/10.1088/1475-7516/2015/07/042 -
Vancouver
Peixoto CJT, Souza V de, Biermann PL. Cosmic rays: the spectrum and chemical composition from '10 POT. 10' to '10 POT. 20' eV [Internet]. Journal of Cosmology and Astroparticle Physics. 2015 ; 2015 42-1-42-12.[citado 2025 dez. 26 ] Available from: https://doi.org/10.1088/1475-7516/2015/07/042 - Probing the radio emission from air showers with polarization measurements
- Study of the impact of different hadronic interactions models in telescope parameters for CTA observatory
- Observation of a large-scale anisotropy in the arrival directions of cosmic rays above 8 × 10 'POT.' 18 eV
- Estimating the Depth of Shower Maximum using the Surface Detectors of the Pierre Auger Observatory
- Composition Classification of Ultra-High Energy Cosmic Rays
- Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America
- Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above '10 POT. 17.8' eV
- Measurement of the proton-air cross section at 's POT. 1/2' = 57 TeV with the Pierre Auger Observatory
- Ultra-high energy neutrinos at the Pierre Auger Observatory
- Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory
Informações sobre o DOI: 10.1088/1475-7516/2015/07/042 (Fonte: oaDOI API)
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