The primary cosmic ray proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the Na- tional Gran Sasso Laboratories by means of EAS-TOP and MACRO detectors. Proton and helium (’p+He’) and proton, helium and CNO (’p+He+CNO’) primaries are selected at 80 TeV, and at 250 TeV respec- tively. Results of this measurement have been interpreted using three different interaction models (QGSJET, SYBILL and DPMJET) inside the CORSIKA framework. Results using all interaction models show a domi- nance of the helium component in the 80-300 TeV region.
Bertaina, M., Stamerra, A., Navarra, G., Battisoni, G., Grillo, A. (2005). A measurement of the proton, helium and CNO fluxes at E0~100 TeV from the EAS- TOP (Cherenkov) and MACRO (TeV Muon) data at the Gran Sasso Laboratories. In Proceedings of the 29th International Cosmic Ray Conference (pp.41-44). B. Sripathi Acharya, Sunil Gupta, P. Jagadeesan, Atul Jain, S. Karthikeyan, Samuel Morris, and Suresh Tonwar.
A measurement of the proton, helium and CNO fluxes at E0~100 TeV from the EAS- TOP (Cherenkov) and MACRO (TeV Muon) data at the Gran Sasso Laboratories
STAMERRA, ANTONIO;
2005-01-01
Abstract
The primary cosmic ray proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the Na- tional Gran Sasso Laboratories by means of EAS-TOP and MACRO detectors. Proton and helium (’p+He’) and proton, helium and CNO (’p+He+CNO’) primaries are selected at 80 TeV, and at 250 TeV respec- tively. Results of this measurement have been interpreted using three different interaction models (QGSJET, SYBILL and DPMJET) inside the CORSIKA framework. Results using all interaction models show a domi- nance of the helium component in the 80-300 TeV region.File | Dimensione | Formato | |
---|---|---|---|
(2005-04)_16041-jap-bertaina-Mario-E-abs1-he11-oral.pdf
non disponibili
Tipologia:
Post-print
Licenza:
NON PUBBLICO - Accesso privato/ristretto
Dimensione
248.52 kB
Formato
Adobe PDF
|
248.52 kB | Adobe PDF | Visualizza/Apri Richiedi una copia |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
https://hdl.handle.net/11365/42930
Attenzione
Attenzione! I dati visualizzati non sono stati sottoposti a validazione da parte dell'ateneo