A Method for energy estimation and mass composition determination of primary cosmic rays at Chacaltaya observation level based on atmospheric Cerenkov light technique

A new method for energy and mass composition estimation of primary cosmic ray radiation based on atmospheric Cerenkov light flux in extensive air showers (EAS) analysis is proposed. The Cerenkov light flux in EAS initiated by primary protons and iron nuclei is simulated with CORSIKA 5.62 code for Ch...

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Detalles Bibliográficos
Autores principales: Mavrodiev, S C, Mishev, A, Stamenov, J N
Lenguaje:eng
Publicado: 2003
Materias:
Astrophysics and Astronomy
Acceso en línea:http://cds.cern.ch/record/678242

Internet

http://cds.cern.ch/record/678242

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