A search for cosmic ray bursts at 0.1 PeV with a small air shower array

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00564471" target="_blank" >RIV/68378271:_____/22:00564471 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/68407700:21670/22:00363706 RIV/47813059:19630/22:A0000198

Výsledek na webu

<a href="https://hdl.handle.net/11104/0336132" target="_blank" >https://hdl.handle.net/11104/0336132</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.3390/sym14030501" target="_blank" >10.3390/sym14030501</a>

Jazyk výsledku

angličtina

Název v původním jazyce

A search for cosmic ray bursts at 0.1 PeV with a small air shower array

Popis výsledku v původním jazyce

The Cosmic Ray Extremely Distributed Observatory (CREDO) pursues a global research strategy dedicated to the search for correlated cosmic rays, so-called Cosmic Ray Ensembles (CRE). Its general approach to CRE detection does not involve any a priori considerations, and its search strategy encompasses both spatial and temporal correlations, on different scales. Here we search for time clustering of the cosmic ray events collected with a small sea-level extensive air shower array at the University of Adelaide. The array consists of seven one-square-metre scintillators enclosing an area of 10 m x 19 m. It has a threshold energy -0.1 PeV, and records cosmic ray showers at a rate of similar to 6 mHz. We have examined event arrival times over a period of over 2.5 years in two equipment configurations (without and with GPS timing), recording similar to 300 k events and similar to 100 k events.

Název v anglickém jazyce

A search for cosmic ray bursts at 0.1 PeV with a small air shower array

Popis výsledku anglicky

The Cosmic Ray Extremely Distributed Observatory (CREDO) pursues a global research strategy dedicated to the search for correlated cosmic rays, so-called Cosmic Ray Ensembles (CRE). Its general approach to CRE detection does not involve any a priori considerations, and its search strategy encompasses both spatial and temporal correlations, on different scales. Here we search for time clustering of the cosmic ray events collected with a small sea-level extensive air shower array at the University of Adelaide. The array consists of seven one-square-metre scintillators enclosing an area of 10 m x 19 m. It has a threshold energy -0.1 PeV, and records cosmic ray showers at a rate of similar to 6 mHz. We have examined event arrival times over a period of over 2.5 years in two equipment configurations (without and with GPS timing), recording similar to 300 k events and similar to 100 k events.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2022

Kód důvěrnosti údajů

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

Název periodika

Symmetry-Basel

ISSN

2073-8994

e-ISSN

2073-8994

Svazek periodika

14

Číslo periodika v rámci svazku

3

Stát vydavatele periodika

CH - Švýcarská konfederace

Počet stran výsledku

10

Strana od-do

501

Kód UT WoS článku

000774608500001

EID výsledku v databázi Scopus

2-s2.0-85126456833