Simulations of Extensive Air Showers triggered by proton, iron and gamma primaries

Geranios, A; Fokitis, E; Maltezos, S; Patrinos, K; Dimopoulos, A

dc.contributor.author	Geranios, A	en
dc.contributor.author	Fokitis, E	en
dc.contributor.author	Maltezos, S	en
dc.contributor.author	Patrinos, K	en
dc.contributor.author	Dimopoulos, A	en
dc.date.accessioned	2014-03-01T02:43:32Z
dc.date.available	2014-03-01T02:43:32Z
dc.date.issued	2005	en
dc.identifier.issn	0217-751X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/31463
dc.subject	AIRES	en
dc.subject	EAS	en
dc.subject	UHECR	en
dc.subject.classification	Physics, Nuclear	en
dc.subject.classification	Physics, Particles & Fields	en
dc.title	Simulations of Extensive Air Showers triggered by proton, iron and gamma primaries	en
heal.type	conferenceItem	en
heal.identifier.primary	10.1142/S0217751X0503017X	en
heal.identifier.secondary	http://dx.doi.org/10.1142/S0217751X0503017X	en
heal.language	English	en
heal.publicationDate	2005	en
heal.abstract	Using the AIRES code, we have generated a large number of Extensive Air Showers corresponding to Ultra high energy cosmic ray gammas, protons and iron nuclei with energy range 1015-1022 eV. These simulations clearly show the different atmospheric depths of the Extensive Air Shower maxima in this energy range. © World Scientific Publishing Company.	en
heal.publisher	WORLD SCIENTIFIC PUBL CO PTE LTD	en
heal.journalName	International Journal of Modern Physics A	en
dc.identifier.doi	10.1142/S0217751X0503017X	en
dc.identifier.isi	ISI:000234702700061	en
dc.identifier.volume	20	en
dc.identifier.issue	29	en
dc.identifier.spage	6814	en
dc.identifier.epage	6816	en