Scaler data from the Pierre Auger Observatory as a proxy of solar activity (2025)
- Authors:
- USP affiliated authors: CATALANI, FERNANDO - EEL ; SOUZA FILHO, LUIZ VITOR DE - IFSC ; SANTOS, EDIVALDO MOURA - IF ; PEIXOTO, CARLOS JOSÉ TODERO - EEL ; OLIVEIRA, CAINÃ DE - IFSC
- Unidades: EEL; IFSC; IF
- DOI: 10.22323/1.501.1370
- Subjects: OBSERVATÓRIOS; ASTROFÍSICA
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Proceedings of Science
- ISSN: 1824-8039
- Volume/Número/Paginação/Ano: v. 501, p. 1370-1-1370-13, Dec. 2025
- Conference titles: International Cosmic Ray Conference - ICRC
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
TARICCO, Carla et al. Scaler data from the Pierre Auger Observatory as a proxy of solar activity. Proceedings of Science. Trieste: Escola de Engenharia de Lorena, Universidade de São Paulo. Disponível em: https://doi.org/10.22323/1.501.1370. Acesso em: 02 mar. 2026. , 2025 -
APA
Taricco, C., Catalani, F., Souza, V. de, Oliveira, C. de, Santos, E. M., & Peixoto, C. J. T. (2025). Scaler data from the Pierre Auger Observatory as a proxy of solar activity. Proceedings of Science. Trieste: Escola de Engenharia de Lorena, Universidade de São Paulo. doi:10.22323/1.501.1370 -
NLM
Taricco C, Catalani F, Souza V de, Oliveira C de, Santos EM, Peixoto CJT. Scaler data from the Pierre Auger Observatory as a proxy of solar activity [Internet]. Proceedings of Science. 2025 ; 501 1370-1-1370-13.[citado 2026 mar. 02 ] Available from: https://doi.org/10.22323/1.501.1370 -
Vancouver
Taricco C, Catalani F, Souza V de, Oliveira C de, Santos EM, Peixoto CJT. Scaler data from the Pierre Auger Observatory as a proxy of solar activity [Internet]. Proceedings of Science. 2025 ; 501 1370-1-1370-13.[citado 2026 mar. 02 ] Available from: https://doi.org/10.22323/1.501.1370 - Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory
- The Pierre Auger Observatory open data
- Scaler rates from the Pierre Auger Observatory: a new proxy of solar activity
- Search for photons above 1018 eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory
- The scintillator surface detector of the Pierre Auger observatory
- Data production and Monte Carlo simulations for the Pierre Auger Observatory
- Determination of the energy scale of cosmic ray measurements using the Auger engineering radio array
- Detection of spaceborne lasers with the Pierre Auger Observatory
- Observation of the shadows of the moon and sun using the Pierre Auger Observatory at an average energy of 7 × 1017 eV
- Monitoring and performance of AugerPrime
Informações sobre o DOI: 10.22323/1.501.1370 (Fonte: oaDOI API)
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