A magnetic spectrometer analysis of ultra high energy cosmic ray arrival directions

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00549486" target="_blank" >RIV/68378271:_____/18:00549486 - isvavai.cz</a>

Result on the web

<a href="https://pos.sissa.it/301/525/pdf" target="_blank" >https://pos.sissa.it/301/525/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.301.0525" target="_blank" >10.22323/1.301.0525</a>

Result language

angličtina

Original language name

A magnetic spectrometer analysis of ultra high energy cosmic ray arrival directions

Original language description

We present a method of identifying bright sources of ultra-high energy cosmic rays (UHECRs) embedded in a diffuse background flux by studying UHECR arrival directions. The technique is applicable to sources that produce several observed events, which exhibit energy ordering in their arrival directions due to coherent deflections caused by the regular component of the Galactic magnetic field. We quantify the efficiency of the method with numerical simulations which take into account the possible uncorrelated values of the extragalactic magnetic fields that the UHECRs might encounter, possible turbulent magnetic fields in our own Galaxy, and in particular the non-uniform exposure of UHECR observatories.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

2018

Confidentiality

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

Article name in the collection

Proceedings of Science

ISBN

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ISSN

1824-8039

e-ISSN

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Number of pages

8

Pages from-to

1-8

Publisher name

Sissa Medilab srl

Place of publication

Trieste

Event location

Busan

Event date

Jul 10, 2017

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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