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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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 <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>Simulations of radio signals produced by ultra-high and extremely high energy neutrino induced cascades in Antarctic ice and lunar regolith</title>
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   <name first="Igor" middle="" last="Zheleznykh"></name>
   <organization>Institute for Nuclear Research of the Russian Academy of Sciences</organization>
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   <title>Dr.</title>
   <name first="Igor" middle="" last="Zheleznykh"></name>
   <organization>Institute for Nuclear Research of the Russian Academy of Sciences</organization>
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   <organization>Kansas University</organization>
   <emailHash>bbf8c0056bad3f2e00e33f45dcf6d57c</emailHash>
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   <title>Dr.</title>
   <name first="Anatoly" middle="" last="Butkevich"></name>
   <organization>Institute for Nuclear Research of the Russian Academy of Sciences</organization>
   <emailHash>3818ccc27bfb9a831157dfc9da3a8aa7</emailHash>
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   <title>Dr.</title>
   <name first="Leonid" middle="" last="Dedenko"></name>
   <organization>Department of Physics, Moscow State University</organization>
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   <title>Dr.</title>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
 </location>
 <startDate>2007-07-09T14:45:00</startDate>
 <endDate>2007-07-09T14:45:00</endDate>
 <abstract>Radio signals produced in ice by electromagnetic cascades with energies up to 
10^15 eV have been calculated. Simulations of cascades were performed using 
the SIMEX Code System. The simulation results in the matrix form, which 
described the charge excess evolution, were used to calculate coherent 
Cherenkov radio field from electromagnetic cascades. Comparison with results 
received in the frameworks of the GEANT-4 Code System was made.

A new algorithm was also developed to simulate radio signals produced by 
extremely high energy (up to 10^21 eV) electron-photon and electron-hadron  
cascades in dense media. The base of the algorithm is a multilevel numerical 
scheme.  The Migdal cross-sections are used to take into account the Landau-
Pomeranchuk-Migdal (LPM) effect. Initially a Monte Carlo approach is used at 
the single particle level. When number of particles in a cascade increases up to 
100-1000  transport equations are used. The main goal  is calculations of the 
source functions – numbers of electrons and photons with low energies ( below 
some threshold energy, which may be chosen as 10 GeV) produced in EHE 
cascade. For these low energy particles, the 3-dimensional cascades should be 
simulated in advance by Monte Carlo method with the use of the GEANT-4 or 
SIMEX codes. The 3-dimensional cascade profiles and signal profiles should be 
estimated and stored in some data base library for maximal CPU efficiency. At 
the last step the lateral and angular distributions of negative and positive 
charges in the EHE cascade can be estimated as a sum of known charge 
distributions in low energy cascades taking into account the source functions. 
Finally, with the use of this sum the radio signal produced in the EHE cascade 
may be estimated.</abstract>
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