THE MASS COMPOSITION OF ULTRA HIGH ENERGY COSMIC RAYS

dc.contributor.author	Grillo, Aurelio F.
dc.date.accessioned	2021-12-01T13:24:22Z
dc.date.available	2021-12-01T13:24:22Z
dc.date.issued	2013
dc.identifier.citation	Acta Polytechnica. 2013, vol. 53, no. A, p. 698-702.
dc.identifier.issn	1210-2709 (print)
dc.identifier.issn	1805-2363 (online)
dc.identifier.uri	http://hdl.handle.net/10467/98671
dc.description.abstract	The status of the Mass Composition measurements of Ultra High Energy Cosmic Rays is presented, with emphasis on the results from the Fluorescence Detector of the Pierre Auger Observatory. Possible consequences of the present measurements are discussed, both on the particle physics and astrophysics aspects.	en
dc.format.mimetype	application/pdf
dc.language.iso	eng
dc.publisher	České vysoké učení technické v Praze	cs
dc.publisher	Czech Technical University in Prague	en
dc.relation.ispartofseries	Acta Polytechnica
dc.relation.uri	https://ojs.cvut.cz/ojs/index.php/ap/article/view/1951
dc.rights	Creative Commons Attribution 4.0 International License	en
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/
dc.title	THE MASS COMPOSITION OF ULTRA HIGH ENERGY COSMIC RAYS
dc.type	article	en
dc.date.updated	2021-12-01T13:24:22Z
dc.identifier.doi	10.14311/AP.2013.53.0698
dc.rights.access	openAccess
dc.type.status	Peer-reviewed
dc.type.version	publishedVersion

Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International License