Detection of Cosmic-Ray Ensembles with CREDO

One of the main objectives of cosmic-ray studies are precise measurements of the energy and chemical composition of particles with extreme energies. Large and sophisticated detectors are used to find events seen as showers starting in the Earth's atmosphere with recorded energies larger than 10...

Full description

Saved in:
Bibliographic Details
Published in:EPJ Web of conferences 2019, Vol.208, p.15006
Main Author: Woźniak, Krzysztof W.
Format: Article
Language:English
Subjects:
Chemical composition
Cosmic rays
Detectors
Organic chemistry
Sensors
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c321t-123bb35c4643a969b3dca54c15a236f9bc801bcddec67984cb93932efecb87493
cites cdi_FETCH-LOGICAL-c321t-123bb35c4643a969b3dca54c15a236f9bc801bcddec67984cb93932efecb87493
container_end_page
container_issue
container_start_page 15006
container_title EPJ Web of conferences
container_volume 208
creator Woźniak, Krzysztof W.
description One of the main objectives of cosmic-ray studies are precise measurements of the energy and chemical composition of particles with extreme energies. Large and sophisticated detectors are used to find events seen as showers starting in the Earth's atmosphere with recorded energies larger than 100 EeV. However, a Cosmic-Ray Ensemble (CRE) developing before reaching the Earth as a bunch of correlated particles may spread over larger areas and requires an extended set of detectors to be discovered. The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a solution to find such phenomena. Even simple detectors measuring the particle arrival time only are useful in this approach, as they are sufficient both to provide candidate CRE events and to determine the direction from which they are arriving.
doi_str_mv 10.1051/epjconf/201920815006
format article
fullrecord <record><control><sourceid>proquest_doaj_</sourceid><recordid>TN_cdi_doaj_primary_oai_doaj_org_article_bb96f56bbbb74c108e57f3c3301bf656</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><doaj_id>oai_doaj_org_article_bb96f56bbbb74c108e57f3c3301bf656</doaj_id><sourcerecordid>2285048453</sourcerecordid><originalsourceid>FETCH-LOGICAL-c321t-123bb35c4643a969b3dca54c15a236f9bc801bcddec67984cb93932efecb87493</originalsourceid><addsrcrecordid>eNpNkFFLwzAUhYMoOOb-gQ8FX61LcpO0eZRu6mAwGAq-hSRNtGVrZtIh-_dWN2Tn5V4uh_NdDkK3BD8QzMnU7VobOj-lmEiKS8IxFhdoRAnGOSbs_fJsv0aTlFo8CKQELkbofuZ6Z_smdFnwWRXStrH5Wh-yeZfc1mxcyr6b_jOr1vPZ6gZdeb1JbnKaY_T2NH-tXvLl6nlRPS5zC5T0OaFgDHDLBAMthTRQW82ZJVxTEF4aW2JibF07KwpZMmskSKDOO2vKgkkYo8Uxtw66VbvYbHU8qKAb9XcI8UPp2Dd245QxUnguzKBiIODS8cKDBRgIXnAxZN0ds3YxfO1d6lUb9rEb3leUlhyzknEYXOzosjGkFJ3_pxKsfmtWp5rVec3wA534b4c</addsrcrecordid><sourcetype>Open Website</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2285048453</pqid></control><display><type>article</type><title>Detection of Cosmic-Ray Ensembles with CREDO</title><source>Publicly Available Content Database</source><source>Free Full-Text Journals in Chemistry</source><creator>Woźniak, Krzysztof W.</creator><contributor>Itow, Y. ; Menjo, H. ; Sako, T. ; Pattison, B.</contributor><creatorcontrib>Woźniak, Krzysztof W. ; Itow, Y. ; Menjo, H. ; Sako, T. ; Pattison, B.</creatorcontrib><description>One of the main objectives of cosmic-ray studies are precise measurements of the energy and chemical composition of particles with extreme energies. Large and sophisticated detectors are used to find events seen as showers starting in the Earth's atmosphere with recorded energies larger than 100 EeV. However, a Cosmic-Ray Ensemble (CRE) developing before reaching the Earth as a bunch of correlated particles may spread over larger areas and requires an extended set of detectors to be discovered. The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a solution to find such phenomena. Even simple detectors measuring the particle arrival time only are useful in this approach, as they are sufficient both to provide candidate CRE events and to determine the direction from which they are arriving.</description><identifier>ISSN: 2100-014X</identifier><identifier>ISSN: 2101-6275</identifier><identifier>EISSN: 2100-014X</identifier><identifier>DOI: 10.1051/epjconf/201920815006</identifier><language>eng</language><publisher>Les Ulis: EDP Sciences</publisher><subject>Chemical composition ; Cosmic rays ; Detectors ; Organic chemistry ; Sensors</subject><ispartof>EPJ Web of conferences, 2019, Vol.208, p.15006</ispartof><rights>2019. This work is licensed under http://creativecommons.org/licenses/by/4.0 (the “License”). Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c321t-123bb35c4643a969b3dca54c15a236f9bc801bcddec67984cb93932efecb87493</citedby><cites>FETCH-LOGICAL-c321t-123bb35c4643a969b3dca54c15a236f9bc801bcddec67984cb93932efecb87493</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2285048453?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>309,310,314,780,784,789,790,4024,23930,23931,25140,25753,27923,27924,27925,37012,44590</link.rule.ids></links><search><contributor>Itow, Y.</contributor><contributor>Menjo, H.</contributor><contributor>Sako, T.</contributor><contributor>Pattison, B.</contributor><creatorcontrib>Woźniak, Krzysztof W.</creatorcontrib><title>Detection of Cosmic-Ray Ensembles with CREDO</title><title>EPJ Web of conferences</title><description>One of the main objectives of cosmic-ray studies are precise measurements of the energy and chemical composition of particles with extreme energies. Large and sophisticated detectors are used to find events seen as showers starting in the Earth's atmosphere with recorded energies larger than 100 EeV. However, a Cosmic-Ray Ensemble (CRE) developing before reaching the Earth as a bunch of correlated particles may spread over larger areas and requires an extended set of detectors to be discovered. The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a solution to find such phenomena. Even simple detectors measuring the particle arrival time only are useful in this approach, as they are sufficient both to provide candidate CRE events and to determine the direction from which they are arriving.</description><subject>Chemical composition</subject><subject>Cosmic rays</subject><subject>Detectors</subject><subject>Organic chemistry</subject><subject>Sensors</subject><issn>2100-014X</issn><issn>2101-6275</issn><issn>2100-014X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><sourceid>DOA</sourceid><recordid>eNpNkFFLwzAUhYMoOOb-gQ8FX61LcpO0eZRu6mAwGAq-hSRNtGVrZtIh-_dWN2Tn5V4uh_NdDkK3BD8QzMnU7VobOj-lmEiKS8IxFhdoRAnGOSbs_fJsv0aTlFo8CKQELkbofuZ6Z_smdFnwWRXStrH5Wh-yeZfc1mxcyr6b_jOr1vPZ6gZdeb1JbnKaY_T2NH-tXvLl6nlRPS5zC5T0OaFgDHDLBAMthTRQW82ZJVxTEF4aW2JibF07KwpZMmskSKDOO2vKgkkYo8Uxtw66VbvYbHU8qKAb9XcI8UPp2Dd245QxUnguzKBiIODS8cKDBRgIXnAxZN0ds3YxfO1d6lUb9rEb3leUlhyzknEYXOzosjGkFJ3_pxKsfmtWp5rVec3wA534b4c</recordid><startdate>2019</startdate><enddate>2019</enddate><creator>Woźniak, Krzysztof W.</creator><general>EDP Sciences</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>DOA</scope></search><sort><creationdate>2019</creationdate><title>Detection of Cosmic-Ray Ensembles with CREDO</title><author>Woźniak, Krzysztof W.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c321t-123bb35c4643a969b3dca54c15a236f9bc801bcddec67984cb93932efecb87493</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Chemical composition</topic><topic>Cosmic rays</topic><topic>Detectors</topic><topic>Organic chemistry</topic><topic>Sensors</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Woźniak, Krzysztof W.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Directory of Open Access Journals</collection><jtitle>EPJ Web of conferences</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Woźniak, Krzysztof W.</au><au>Itow, Y.</au><au>Menjo, H.</au><au>Sako, T.</au><au>Pattison, B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Detection of Cosmic-Ray Ensembles with CREDO</atitle><jtitle>EPJ Web of conferences</jtitle><date>2019</date><risdate>2019</risdate><volume>208</volume><spage>15006</spage><pages>15006-</pages><issn>2100-014X</issn><issn>2101-6275</issn><eissn>2100-014X</eissn><abstract>One of the main objectives of cosmic-ray studies are precise measurements of the energy and chemical composition of particles with extreme energies. Large and sophisticated detectors are used to find events seen as showers starting in the Earth's atmosphere with recorded energies larger than 100 EeV. However, a Cosmic-Ray Ensemble (CRE) developing before reaching the Earth as a bunch of correlated particles may spread over larger areas and requires an extended set of detectors to be discovered. The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a solution to find such phenomena. Even simple detectors measuring the particle arrival time only are useful in this approach, as they are sufficient both to provide candidate CRE events and to determine the direction from which they are arriving.</abstract><cop>Les Ulis</cop><pub>EDP Sciences</pub><doi>10.1051/epjconf/201920815006</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 2100-014X
ispartof EPJ Web of conferences, 2019, Vol.208, p.15006
issn 2100-014X
2101-6275
2100-014X
language eng
recordid cdi_doaj_primary_oai_doaj_org_article_bb96f56bbbb74c108e57f3c3301bf656
source Publicly Available Content Database; Free Full-Text Journals in Chemistry
subjects Chemical composition
Cosmic rays
Detectors
Organic chemistry
Sensors
title Detection of Cosmic-Ray Ensembles with CREDO
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-03T18%3A13%3A32IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_doaj_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Detection%20of%20Cosmic-Ray%20Ensembles%20with%20CREDO&rft.jtitle=EPJ%20Web%20of%20conferences&rft.au=Wo%C5%BAniak,%20Krzysztof%20W.&rft.date=2019&rft.volume=208&rft.spage=15006&rft.pages=15006-&rft.issn=2100-014X&rft.eissn=2100-014X&rft_id=info:doi/10.1051/epjconf/201920815006&rft_dat=%3Cproquest_doaj_%3E2285048453%3C/proquest_doaj_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c321t-123bb35c4643a969b3dca54c15a236f9bc801bcddec67984cb93932efecb87493%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2285048453&rft_id=info:pmid/&rfr_iscdi=true