Cosmic-Ray Extremely Distributed Observatory: Status and Perspectives
- NázevTitle
- Cosmic-Ray Extremely Distributed Observatory: Status and PerspectivesCosmic-Ray Extremely Distributed Observatory: Status and Perspectives
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- D. Gora, K. Cheminant, D. Alvarez-Castillo, L. Bratek, K. Smolek
- Klíčová slovaKeywords
- energy photon propagation, simulation
- KonferenceConference
- 7th International Conference on New Frontiers in Physics (Kolymbari, Greece, 2018-07-04)
- DOIDOI
- 10.3390/universe4110111
- Časopis / citaceJournal / citation
- Universe 4(11), 111 (2018) · ISSN 2218-1997
- RokYear
- 2018
- JazykLanguage
- eng
- ZáznamyRecords
- ProjektProject
- Inženýrské aplikace fyziky mikrosvětaEngineering applications of microworld physics
- CitovánoCited by
- 12 (INSPIRE-HEP)
- Plný text (open access)Full text (open access)
- https://www.mdpi.com/2218-1997/4/11/111/pdf?version=1541643324
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
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 overspread a significant fraction of the Earth, is a scientific terra incognita. Instead of developing and commissioning a completely new global detector infrastructure, CREDO proposes approaching the global cosmic-ray analysis objectives with all types of available detectors, from professional to pocket size, merged into a worldwide network. With such a network it is possible to search for evidences of correlated cosmic-ray ensembles. One of the observables that can be investigated in CREDO is a number of spatially isolated events collected in a small time window which could shed light on fundamental physics issues. The CREDO mission and strategy requires active engagement of a large number of participants, also non-experts, who will contribute to the project by using common electronic devices (e.g., smartphones). In this note, the status and perspectives of the project are presented.
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 overspread a significant fraction of the Earth, is a scientific terra incognita. Instead of developing and commissioning a completely new global detector infrastructure, CREDO proposes approaching the global cosmic-ray analysis objectives with all types of available detectors, from professional to pocket size, merged into a worldwide network. With such a network it is possible to search for evidences of correlated cosmic-ray ensembles. One of the observables that can be investigated in CREDO is a number of spatially isolated events collected in a small time window which could shed light on fundamental physics issues. The CREDO mission and strategy requires active engagement of a large number of participants, also non-experts, who will contribute to the project by using common electronic devices (e.g., smartphones). In this note, the status and perspectives of the project are presented.