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A measurement of the average longitudinal development profile of cosmic ray air showers between 1017 and 1018 eV

T Abu-Zayyad,K Belov,D.J Bird,J Boyer,Z Cao,M Catanese,G.F Chen,R.W Clay,C.E Covault,H.Y Dai,B.R Dawson,J.W Elbert,B.E Fick,L.F Fortson,J.W Fowler,K.G Gibbs,M.A.K Glasmacher,K.D Green,Y Ho,A Huang,C.C Jui,M.J Kidd,D.B Kieda,B.C Knapp,S Ko,C.G Larsen,W Lee,E.C Loh,E.J Mannel,J Matthews,J.N Matthews,B.J Newport,D.F Nitz,R.A Ong,K.M Simpson, J.D Smith,D Sinclair,P Sokolsky,C Song,J.K.K Tang,S.B Thomas,J.C van der Velde,L.R Wiencke,C.R Wilkinson, S Yoshida,X.Z Zhang

Astroparticle Physics（2001）

Cited 78|Views58
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Abstract
The average extensive air shower longitudinal development profile is measured. Events between 1017 and 1018 eV recorded by the HiRes/MIA hybrid experiment are used for the average profile. Several functional forms are examined using this average profile. The best-fit parameters for the above functions are determined.
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96.40.Pq,98.70.Sa,13.85.Tp
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