3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
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Contribution Poster (WITHDRAWN)
HE.1.4.B
Towards the estimate of sensitivity of Telescope Array to chemical composition of cosmic rays
Speakers
- Dr. Dmitry GORBUNOV
Primary authors
- Dr. Dmitry GORBUNOV (INR RAS)
Co-authors
- Dr. Grigory RUBTSOV (INR RAS)
- Dr. Sergey TROITSKY (INR RAS)
Abstract content
We use a public available library of extensive air showers simulated without thinning for the realistic setup of Telescope Array experiment (TA) to outline the distributions of observables available at ground array part of TA. These distributions are analysed to estimate the size of physical fluctuations which allows to choose the observables most sensitive to energy and chemical composition of cosmic ray primaries. Preliminary results will be presented at the conference.