The evolution of the moments of the 'X IND. max' distribution with energy and primary particle mass (2011)
- Author:
- USP affiliated author: SOUZA FILHO, LUIZ VITOR DE - IFSC
- School: IFSC
- Subjects: ASTROFÍSICA; RAIOS CÓSMICOS (ESTUDO;COMPARAÇÃO)
- Language: Inglês
- Imprenta:
- Publisher: International Union of Pure and Applied Physics - IUPAP
- Place of publication: London
- Date published: 2011
- Source:
- Título do periódico: Proceedings
- Conference title: International Cosmic Ray Conference - ICRC
-
ABNT
SOUZA, Vitor de. The evolution of the moments of the 'X IND. max' distribution with energy and primary particle mass. 2011, Anais.. London: International Union of Pure and Applied Physics - IUPAP, 2011. . Acesso em: 02 jul. 2022. -
APA
Souza, V. de. (2011). The evolution of the moments of the 'X IND. max' distribution with energy and primary particle mass. In Proceedings. London: International Union of Pure and Applied Physics - IUPAP. -
NLM
Souza V de. The evolution of the moments of the 'X IND. max' distribution with energy and primary particle mass. Proceedings. 2011 ;[citado 2022 jul. 02 ] -
Vancouver
Souza V de. The evolution of the moments of the 'X IND. max' distribution with energy and primary particle mass. Proceedings. 2011 ;[citado 2022 jul. 02 ] - A new analysis of the combined data from both KASCADE and KASCADE-Grande
- Autonomous RPCs for a cosmic ray ground array
- A new release of the KASCADE Cosmic Ray Data Centre (KCDC)
- Muon density measurements for the light and heavy mass groups of cosmic rays at the KASCADE-Grande observatory
- Measurements of the depth of maximum of air-shower profiles at the Pierre Auger observatory and their composition implications
- Preliminary studies of the effect of thinning techniques over muon production profiles
- LOPES: recent results and open questions on the radio detection of air showers
- A limit on the diffuse gamma-rays measured with KASCADE-Grande
- All-particle energy spectrum of KASCADE-Grande based on shower size and different hadronic interaction models
- The composition of UHECRs studied with the fluorescence detector of the Pierre Auger Observatory
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