Determination of cosmic-ray primary mass on an event-by-event basis using radio detection (2019)
- Authors:
- Autor USP: CARVALHO JUNIOR, WASHINGTON RODRIGUES DE - IF
- Unidade: IF
- DOI: 10.1016/j.astropartphys.2019.02.005
- Subjects: ASTROFÍSICA; COSMOLOGIA; RAIOS CÓSMICOS; RADIOASTRONOMIA
- Keywords: Ultra-high energy cosmic rays; Extensive air showers; Radio emission; Mass composition
- Agências de fomento:
- Language: Português
- Imprenta:
- Source:
- Título: Astroparticle Physics
- ISSN: 0927-6505
- Volume/Número/Paginação/Ano: v. 109, p. 41-49, maio 2019
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
- Licença: cc-by
-
ABNT
CARVALHO JR., Washington e ALVAREZ-MUÑIZ, Jaime. Determination of cosmic-ray primary mass on an event-by-event basis using radio detection. Astroparticle Physics, v. 109, p. 41-49, 2019Tradução . . Disponível em: https://doi.org/10.1016/j.astropartphys.2019.02.005. Acesso em: 05 jan. 2026. -
APA
Carvalho Jr., W., & Alvarez-Muñiz, J. (2019). Determination of cosmic-ray primary mass on an event-by-event basis using radio detection. Astroparticle Physics, 109, 41-49. doi:10.1016/j.astropartphys.2019.02.005 -
NLM
Carvalho Jr. W, Alvarez-Muñiz J. Determination of cosmic-ray primary mass on an event-by-event basis using radio detection [Internet]. Astroparticle Physics. 2019 ; 109 41-49.[citado 2026 jan. 05 ] Available from: https://doi.org/10.1016/j.astropartphys.2019.02.005 -
Vancouver
Carvalho Jr. W, Alvarez-Muñiz J. Determination of cosmic-ray primary mass on an event-by-event basis using radio detection [Internet]. Astroparticle Physics. 2019 ; 109 41-49.[citado 2026 jan. 05 ] Available from: https://doi.org/10.1016/j.astropartphys.2019.02.005 - Prospects for high-elevation radio detection of >100 PeV tau neutrinos
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- Radio interferometry applied to the observation of cosmic-ray induced extensive air showers
- Erratum to “The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory” [Astroparticle Physics 35 (2011) 266–276]
- Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory
- Erratum to “The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory” [Astroparticle Physics 35 (2011) 266–276]
- The lateral trigger probability function for the ultra-high energy cosmic ray showers detected by the Pierre Auger Observatory
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Informações sobre o DOI: 10.1016/j.astropartphys.2019.02.005 (Fonte: oaDOI API)
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