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Possible composition of the primary particles at ultrahigh energies observed at the Yakutsk array

Possible composition of the primary particles at ultrahigh energies observed at the Yakutsk array

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1730079126

Possible composition of the primary particles at ultrahigh energies observed at the Yakutsk array

About this item

Full title

Possible composition of the primary particles at ultrahigh energies observed at the Yakutsk array

Publisher

Bristol: IOP Publishing

Journal title

Journal of physics. Conference series, 2013-01, Vol.409 (1), p.12068-4

Language

English

Formats

Publication information

Publisher

Bristol: IOP Publishing

More information

Scope and Contents

Contents

The composition of the primary cosmic radiation should be studied by various alternative approaches. A promising way is to exploit a dependence of the fraction of muons in an extensive air shower on the atomic number of the primary nuclei. A comparison of the fraction of muons at 600 m from the shower axis observed at the Yakutsk array in the verti...

Alternative Titles

Full title

Possible composition of the primary particles at ultrahigh energies observed at the Yakutsk array

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_1730079126

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1730079126

Other Identifiers

ISSN

1742-6596,1742-6588

E-ISSN

1742-6596

DOI

10.1088/1742-6596/409/1/012068

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