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Estimat eo fth eCosmi cRa yComposition b y aPatter nAnalysi so fth eCor eo fPe VEAS

A. Haungs,T. Anton,W. D. Ape,A. F. Bade,K. Bek,E. Bollman,H. Bozdo,I. M. Brancus,A. Chilingarian,K. Daumiller,P. Dol,J. Engle,F. Feßle r,H. J. Gils,R. Glasstetter,R. Haeusle,W. Hafeman,D. Heck, J. R. H ¨ orandel,T. Hols,K.-H. Kampert,H. Keim,J. Kemp, H. O. Klage,J. Knapp,H. J. Mathe,H. J. Maye r,H. Rebel,M. Risse,M. Rot,G. Schat,F. K. Schmidt,T. Thou,H. Ulrich,A. Vardanyan,J. H. Weber,J. Went,T. Wibig,T. Wieger,D. Wochel,S. Zagromski,Nationa lInstitut,Romania Cosmi

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Abstract
Asyste mo flarge-are apositio nsensitiv emultiwir eproportiona lchamber s(MWPC) ,installe dbelo wthe hadro ncalorimete ro fth eKASCAD E(KArlsruh eShowe rCor ean dArra yDEtector )centra ldetecto ri sabl eto observ eth edensit ydistribution so fth ehig henerg ymuon san dhadron spenetratin gth ecalorimeter .B yus eof aclassificatio ni nterm so fmultifracta lmoments , amas ssensitiv eparametrisatio no fth edensit ydistributions i sgiven .I ncombinatio nwit hadditiona lmeasure dparameters ,i.e .numbe ro freconstructe dmuon si nth ecore an dth eshowe rsiz ea nartificia lneura lne tanalysi slead st oa nestimatio no fth erelativ eabundance so fthe differen tprimar ycomponent si ncosmi cray si nth eenerg yregio naroun dth e"knee".
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