D. Góra, K. A. Cheminant, D. A. Castillo, D. Beznosko, N. Dhital, A. Duffy, P. Homola, K. Kopanski, P. Kovács, Marta Marek, A. Mozgova, V. Nazari, Michal Niedzwiecki, W. Noga, K. Smelcerz, K. Smolek, J. Stasielak, O. Sushchov, D. Ostrogorski, K. Rzecki, Krzysztof W. Woźniak, J. Zamora-Saá
{"title":"Cosmic Ray Extremely Distributed Observatory: Status and Perspectives of a Global Cosmic Ray Detection Framework","authors":"D. Góra, K. A. Cheminant, D. A. Castillo, D. Beznosko, N. Dhital, A. Duffy, P. Homola, K. Kopanski, P. Kovács, Marta Marek, A. Mozgova, V. Nazari, Michal Niedzwiecki, W. Noga, K. Smelcerz, K. Smolek, J. Stasielak, O. Sushchov, D. Ostrogorski, K. Rzecki, Krzysztof W. Woźniak, J. Zamora-Saá","doi":"10.22323/1.358.0272","DOIUrl":null,"url":null,"abstract":"The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to global studies of extremely extended cosmic-ray phenomena, the cosmic-ray ensembles (CRE), beyond the capabilities of existing detectors and observatories. Up to date cosmic-ray research has been focused on detecting single air showers, while the search for ensembles of cosmic-rays, which may spread over a significant fraction of the Earth, is a scientific terra incognita. The key idea of CREDO is to combine existing cosmic-ray detectors (large professional arrays, educational instruments, individual detectors, such as smartphones, etc.) into a worldwide network, thus enabling a global analysis. The second goal of CREDO involves a large number of participants (citizen science!), assuring the geographical spread of the detectors and managing manpower necessary to deal with vast amount of data to search for evidence for cosmic-ray ensembles. In this paper the status and perspectives of the project are presented.","PeriodicalId":166008,"journal":{"name":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","volume":"54 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2019-08-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.22323/1.358.0272","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to global studies of extremely extended cosmic-ray phenomena, the cosmic-ray ensembles (CRE), beyond the capabilities of existing detectors and observatories. Up to date cosmic-ray research has been focused on detecting single air showers, while the search for ensembles of cosmic-rays, which may spread over a significant fraction of the Earth, is a scientific terra incognita. The key idea of CREDO is to combine existing cosmic-ray detectors (large professional arrays, educational instruments, individual detectors, such as smartphones, etc.) into a worldwide network, thus enabling a global analysis. The second goal of CREDO involves a large number of participants (citizen science!), assuring the geographical spread of the detectors and managing manpower necessary to deal with vast amount of data to search for evidence for cosmic-ray ensembles. In this paper the status and perspectives of the project are presented.