A new method for reconstructing the muon lateral distribution with an array of segmented counters

Although the origin of ultra high energy cosmic rays is still unknown, significant progress has been achieved in last decades with the construction of large arrays that are currently taking data. One of the most important pieces of information comes from the chemical composition of primary particles...

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Detalles Bibliográficos
Autores principales: Ravignani, D., Supanitsky, A.D.
Formato: JOUR
Materias:
Cosmic ray primary mass composition
Lateral distribution function
Muon counters
Ultra-high energy cosmic rays
Charged particles
Cosmic ray measurement
Cosmology
Distribution functions
Chemical compositions
Lateral distributions
Primary mass
Primary particles
Reconstruction method
Statistical uncertainty
Systematic uncertainties
Ultra high-energy cosmic rays
Cosmic rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_09276505_v65_n_p1_Ravignani
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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