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  <organization>ICN-UNAM</organization>
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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>
<location>
 <name>Merida, Mexico</name>
 <address></address>
 <room></room>
</location>
<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
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 <user>
  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <title>Study of small scale fluctuations in charged particle and muon densities at the ground level with no-thinning simulations of extensive air showers</title>
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   <title>Mr.</title>
   <name first="Grigory" middle="" last="Rubtsov"></name>
   <organization>Institute for Nuclear Research of the Russian Academy of Sciences</organization>
   <emailHash>854f5555b6210a129935c7d9ca4b0a90</emailHash>
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   <title>Mr.</title>
   <name first="Grigory" middle="" last="Rubtsov"></name>
   <organization>Institute for Nuclear Research of the Russian Academy of Sciences</organization>
   <emailHash>854f5555b6210a129935c7d9ca4b0a90</emailHash>
  </user>
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  <user>
   <title>Dr.</title>
   <name first="Dmitry" middle="" last="Gorbunov"></name>
   <organization>Institute for Nuclear Research of the Russian Academy of Sciences</organization>
   <emailHash>e8edb4a4e881b932ec9111cc8e122bd8</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Vadim" middle="" last="Kuzmin"></name>
   <organization>Institute for Nuclear Research of the Russian Academy of Sciences</organization>
   <emailHash>f7dca3d44401c875e68c44d0ecedb361</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Sergey" middle="" last="Troitsky"></name>
   <organization>Institute for Nuclear Research of the Russian Academy of Sciences</organization>
   <emailHash>7b52e857ba2004d135cf05639f5fcfde</emailHash>
  </user>
 </coAuthors>
 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Kabah (Holiday Inn)</room>
 </location>
 <startDate>2007-07-05T10:30:00</startDate>
 <endDate>2007-07-05T10:42:00</endDate>
 <duration>00:12</duration>
 <abstract>The particle density in extensive air showers fluctuates at the ground level. These
fluctuations, at the scale of the scintillator detector size (several meters), lead
to the diversity of the individual detector responses. Therefore, small scale
fluctuations contribute to the error in the estimation of the primary energy by a
ground array. As a results of analysis of simulated full (unthinned) showers, this
contribution is shown to be non-Gaussian. The impact on the primary energy spectrum
measured by a ground array is estimated. It is argued that super-GZK events observed
by AGASA experiment do not result from the energy overestimation, due to small scale
fluctuations, of lower energy events. We confirmed that the muon density at the
individual muon detectors obeys the Poisson law. The impact of the fluctuations on
the reconstructed muon density at 1000 meters is estimated.</abstract>
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