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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>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
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  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <board>031 (2A)</board>
 <track>HE.1.6</track>
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 <title>A GEANT-based package for determination of the PAMIR experiment X-ray emulsion chamber response</title>
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   <name first="Rauf" middle="" last="Mukhamedshin"></name>
   <organization>Institute for Nuclear Research of Russian Academy of Science</organization>
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   <title>Prof.</title>
   <name first="Rauf" middle="" last="Mukhamedshin"></name>
   <organization>Institute for Nuclear Research of Russian Academy of Science</organization>
   <emailHash>5323daddbb7ae894c7dc96a484995aeb</emailHash>
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   <name first="Konstantin" middle="" last="Kotelnikov"></name>
   <organization>P.N.Lebedev Physical Institute, Russian Academy of Science, Moscow, Russia</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
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   <title></title>
   <name first="Vitaly" middle="" last="Puchkov"></name>
   <organization>P.N.Lebedev Physical Institute, Russian Academy of Science, Moscow, Russia</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
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   <title>Prof.</title>
   <name first="Vladimir" middle="" last="Galkin"></name>
   <organization>D.V.Skobel’tsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
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   <title>Dr.</title>
   <name first="Sergei" middle="" last="Nazarov"></name>
   <organization>D.V.Skobel’tsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
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   <title>Dr.</title>
   <name first="Alexander" middle="" last="Borisov"></name>
   <organization>P.N.Lebedev Physical Institute, Russian Academy of Science, Moscow, Russia</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
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   <title>Dr.</title>
   <name first="Mikhail" middle="" last="Kogan"></name>
   <organization>P.N.Lebedev Physical Institute, Russian Academy of Science, Moscow, Russia</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
 </location>
 <startDate>2007-07-06T14:45:00</startDate>
 <endDate>2007-07-06T14:45:00</endDate>
 <abstract>Analysis of various data accumulated in X-ray emulsion chamber experiments,
especially, data on gamma-ray–hadron families with unusual characteristics
(Centauros, aligned events etc.), requires a comprehensive program to simulate the
propagation of electromagnetic and various-type hadron particles through
sandwich-like media of emulsion chambers as well as measuring procedures used for
emulsion chamber data processing. Such a new computer code ECSim 2.0 has been
recently elaborated on basis of the GEANT 3.21 package. As compared to the latter,
the ECSim 2.0 takes into account the LPM effect for gamma-rays and electrons, uses
new cross sections of muon interactions of different types allowing also for the LPM
effect in pair generation, incorporates QGSJET model for simulation of high-energy
hadron interactions and accounts for production and interactions of charm particles.
Besides, measuring and data treatment procedures employed in the Pamir experiment are
simulated properly. Main features of the ECSim 2.0 code and some results obtained for
the Pamir emulsion chamber experiment are discussed. The ECSim 2.0 can be used widely
for data analysis in various X-ray emulsion chamber experiments.</abstract>
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