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<supportEmail caption="Support">icrc2007@icrc2007.unam.mx</supportEmail>
<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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<closed>True</closed>
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 <name>Merida, Mexico</name>
 <address></address>
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<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
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  <organization>IGeof-UNAM</organization>
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 <title>Towards the estimate of sensitivity of Telescope Array to chemical composition of cosmic rays</title>
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   <title>Dr.</title>
   <name first="Dmitry" middle="" last="Gorbunov"></name>
   <organization>INR RAS</organization>
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   <title>Dr.</title>
   <name first="Dmitry" middle="" last="Gorbunov"></name>
   <organization>INR RAS</organization>
   <emailHash>e8edb4a4e881b932ec9111cc8e122bd8</emailHash>
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   <name first="Grigory" middle="" last="Rubtsov"></name>
   <organization>INR RAS</organization>
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   <organization>INR RAS</organization>
   <emailHash>7b52e857ba2004d135cf05639f5fcfde</emailHash>
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 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
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 <abstract>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.</abstract>
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