Method for studying the chemical composition of the primary cosmic radiation at and above 10/sup 17/eV
Journal Article
·
· JETP Lett. (Engl. Transl.); (United States)
OSTI ID:6289574
A new method is proposed for studying the chemical composition of the primary cosmic radiation. In this method the flux of high-energy muons and the intensity of the Cerenkov radiation of extensive air showers would be measured simultaneously, and the shape of the Cerenkov pulse would be used to fix the shower maximum.
- Research Organization:
- Institute of Nuclear Physics, M. V. Lomonosov Moscow State University
- OSTI ID:
- 6289574
- Journal Information:
- JETP Lett. (Engl. Transl.); (United States), Journal Name: JETP Lett. (Engl. Transl.); (United States) Vol. 33:4; ISSN JTPLA
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640101* -- Astrophysics & Cosmology-- Cosmic Radiation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CHEMICAL COMPOSITION
CHERENKOV RADIATION
COSMIC RADIATION
COSMIC SHOWERS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
ENERGY RANGE
EXTENSIVE AIR SHOWERS
FERMIONS
IONIZING RADIATIONS
LEPTONS
MUONS
PEV RANGE
PRIMARY COSMIC RADIATION
RADIATIONS
SECONDARY COSMIC RADIATION
SHOWERS
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CHEMICAL COMPOSITION
CHERENKOV RADIATION
COSMIC RADIATION
COSMIC SHOWERS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
ENERGY RANGE
EXTENSIVE AIR SHOWERS
FERMIONS
IONIZING RADIATIONS
LEPTONS
MUONS
PEV RANGE
PRIMARY COSMIC RADIATION
RADIATIONS
SECONDARY COSMIC RADIATION
SHOWERS