Published March 1999 | Version v1
Journal article

On the possibility of PCR chemical composition study by means of emulsion chambers

Description

Chemical composition of PCR were investigated by means of emulsion chambers in several works. The conclusion was that the fraction of Fe induced families is less than 3% - 7% and heavy nuclei in primary cosmic rays with energy more than 1016 eV are less than 0.22 - 0.27. The aim of the present report is to show the origin of sensitivity of γ-hadron families to the atomic number of PCR and review once more the conclusion about normal composition of PCR in the energy interval 1015 - 1016 eV

Additional details

Identifiers

PII
S0920563299002364;

Publishing Information

Journal Title
Nuclear Physics. B, Proceedings Supplements
Journal Volume
75
Journal Issue
1-2
Journal Page Range
p. 180-182
ISSN
0920-5632
CODEN
NPBSE7

Conference

Title
10. international symposium on very high energy cosmic ray interactions
Dates
12-17 Jul 1998
Place
Assergi (Italy)

INIS

Country of Publication
Netherlands
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
34060164
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CHEMICAL COMPOSITION; COSMIC PHOTONS; COSMIC RAY DETECTION; NUCLEAR EMULSIONS; PRIMARY COSMIC RADIATION
Descriptors DEC
BOSONS; COSMIC RADIATION; DETECTION; ELEMENTARY PARTICLES; IONIZING RADIATIONS; MASSLESS PARTICLES; PHOTONS; RADIATION DETECTION; RADIATIONS

Optional Information

Copyright
Copyright (c) 1999 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.