A New Study On The Energy Spectrum And Composition Of Primary Cosmic Ray Flux At Energies Similar To 10(14)-10(16) Ev Using The Grapes-3 Array At Ooty

Data collected with the 217-detector air shower array and the 560 m(2) area tracking muon detector, being operated at Ooty in southern India by the India-Japan (Tata Institute-Osaka City University) collaboration, GRAPES, have been analyzed to study the shape of the energy spectrum and the composition around the knee. It is shown that the muon multiplicity distribution, observed with the highly modular muon detector, permits a relatively reliable measurement on the composition of primary flux which then helps in a more accurate reconstruction of the energy spectrum from the observed shower size spectrum. The highlights of the GRAPES array, the analysis procedure and the results are presented.