Report of the working group on the composition of ultra high energy cosmic rays

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F16%3A00551370" target="_blank" >RIV/68378271:_____/16:00551370 - isvavai.cz</a>

Result on the web

<a href="https://journals.jps.jp/doi/pdf/10.7566/JPSCP.9.010016" target="_blank" >https://journals.jps.jp/doi/pdf/10.7566/JPSCP.9.010016</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.7566/JPSCP.9.010016" target="_blank" >10.7566/JPSCP.9.010016</a>

Result language

angličtina

Original language name

Report of the working group on the composition of ultra high energy cosmic rays

Original language description

For the first time a proper comparison of the average depth of shower maximum (Xmax) published by the Pierre Auger and Telescope Array Observatories is presented. The Xmax distributions measured by the Pierre Auger Observatory were fit using simulated events initiated by four primaries (proton, helium, nitrogen and iron). The primary abundances which best describe the Auger data were simulated through the Telescope Array (TA) Middle Drum (MD) fluorescence and surface detector array. The simulated events were analyzed by the TA Collaboration using the same procedure as applied to their data.n

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

—

OECD FORD branch

10303 - Particles and field physics

Project

—

Continuities

—

Publication year

2016

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

JPS Conference Proceedings

ISBN

978-4-89027-113-9

ISSN

2435-3892

e-ISSN

—

Number of pages

7

Pages from-to

1-7

Publisher name

Physical Society of Japan

Place of publication

Tokyo

Event location

Springdale, Utah

Event date

Oct 12, 2014

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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