A method of searching for origins of cosmic rays correcting for galactic field deflections and charge composition

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00550834" target="_blank" >RIV/68378271:_____/18:00550834 - isvavai.cz</a>

Result on the web

<a href="https://pos.sissa.it/301/518/pdf" target="_blank" >https://pos.sissa.it/301/518/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.301.0518" target="_blank" >10.22323/1.301.0518</a>

Result language

angličtina

Original language name

A method of searching for origins of cosmic rays correcting for galactic field deflections and charge composition

Original language description

We present a new method of searching for origins of ultra-high energy cosmic rays directly from observed data. We include corrections for deflections in the galactic magnetic field according to the individual cosmic ray charges. The analysis procedure is iterative and consists of the following steps. Initially, we assign to each cosmic ray a charge hypothesis and apply corresponding corrections for the galactic field to obtain directions outside our galaxy. We then search for directions indicating an enhanced cosmic ray arrival probability using a clustering algorithm. The cluster directions form a set of source candidates.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

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Continuities

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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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