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[en] An indirect approach to deduce the elongation rate De and the fluctuations of the atmospheric depth Xm of the EAS maximum from muon arrival time distributions has been scrutinized on basis of Monte Carlo simulations of the EAS development and of the longitudinal profile of various EAS parameters. Special attention is made to the behaviour of a scaling parameter relating the variations at the height of the shower maximum to the arrival time of muons at observation level. (orig.)
Source
Chilingarian, A.A.; Sanosyan, Kh.N. (Erevanskij Fizicheskij Inst., Erevan (Armenia). Cosmic Ray Dept.) (eds.); Haungs, A.; Rebel, H.; Forschungszentrum Karlsruhe GmbH Technik und Umwelt (Germany). Inst. fuer Kernphysik; 148 p; ISSN 0947-8620; 
; May 2000; p. 133-137; Workshop ANI 99 - Current topics of cosmic ray research with EAS observations; Yerevan (Armenia); 29 May - 3 Jun 1999; Available from TIB Hannover: ZA 5141(6472)
; May 2000; p. 133-137; Workshop ANI 99 - Current topics of cosmic ray research with EAS observations; Yerevan (Armenia); 29 May - 3 Jun 1999; Available from TIB Hannover: ZA 5141(6472)