20.500.12556/RUNG-2159
Report of the Working Group on the Composition of Ultra-High Energy Cosmic Rays
The atmospheric depth, Xmax, at which the particle number of
an air shower reaches its maximum is a good indicator for the
mass of the primary particle. We present a comparison of the
energy evolution of the mean of Xmax as measured by the
Telescope Array and c Collaborations. After
accounting for the different resolutions, acceptances and
analysis strategies of the two experiments, the two results are
found to be in good agreement within systematic uncertainties.
Pierre Auger Observatory
Telescope Array
Ultra-High Energy Cosmic Rays
elemental composition
extensive air showers
the atmospheric depth of the air shower maximum
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Angleški jezik
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2016-03-08 14:40:16
2016-03-08 15:13:07
2023-06-09 03:15:51
0000-00-00 00:00:00
2015
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4158459
URN:SI:UNG:REP:CV0X6NRC
ICRC2015_307.pdf
ICRC2015_307.pdf
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a4663f2cbc6532506c226b0b765a07c6b3b76081c2c6d5926e027b1652c8f928
defd7f0b-05cd-11ee-9c48-5ef991fed68f
https://repozitorij.ung.si/Dokument.php?lang=slv&id=3597
Univerza v Novi Gorici
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