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  <organization>ICN-UNAM</organization>
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  <userid>3</userid>
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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>
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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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 <track>HE.1.6</track>
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  <name>Oral</name>
 </type>
 <title>Testing the low energy hadronic models used in Aires, with CAPRICE98 results.</title>
 <speakers>
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   <title>Dr.</title>
   <name first="Patricia Maria" middle="" last="Hansen"></name>
   <organization>Departamento de Fisica de Particulas -Universidade de Santiago de Compostela-15782 Santiago de Compostela,Spain</organization>
   <emailHash>3d96cf773231cd29509730d0f336af91</emailHash>
  </user>
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   <title>Dr.</title>
   <name first="Patricia Maria" middle="" last="Hansen"></name>
   <organization>Departamento de Fisica de Particulas -Universidade de Santiago de Compostela-15782 Santiago de Compostela,Spain</organization>
   <emailHash>3d96cf773231cd29509730d0f336af91</emailHash>
  </user>
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   <title>Dr.</title>
   <name first="Sergio J" middle="" last="Sciutto"></name>
   <organization>Departamento de Fisica -Universidad Nacional de La Plata-Universidad de La Plata-Argentina</organization>
   <emailHash>1ee7d922f5fa26b271326ea3df6318b6</emailHash>
  </user>
  <user>
   <title>Prof.</title>
   <name first="Per" middle="" last="Carlson"></name>
   <organization>Royal Institute of Technology (KTH),AlbaNova University Center,S-10681Stockholm Sweden</organization>
   <emailHash>92cf9a36947b59aa94a9af8ba55f1874</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Mirko" middle="" last="Boezio"></name>
   <organization>Sezione INFN di Trieste, 34127 Trieste, Italy.</organization>
   <emailHash>d96364df861cf14ba8d89ef7ec5c4000</emailHash>
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  <user>
   <title>Dr.</title>
   <name first="Emiliano" middle="" last="Mocchiutti"></name>
   <organization>Sezione INFN di Trieste, 34127 Trieste, Italy.</organization>
   <emailHash>a8f5e5c57fefb89cc933d8ee5a753459</emailHash>
  </user>
 </coAuthors>
 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Kabah (Holiday Inn)</room>
 </location>
 <startDate>2007-07-05T10:54:00</startDate>
 <endDate>2007-07-05T11:06:00</endDate>
 <duration>00:12</duration>
 <abstract>Air shower simulation programs are used to reconstruct the energy in the UHECR
surface detectors. This reconstruction is based on the lateral distribution function
obtained in the experiment. It is also known that this function at core distance
greater than 1 km strongly depends on the low energy hadronic models used in the
simulation. There are discrepancies in the particle production
due to the different models that are used. This discrepancy is not only at high 
(&gt;100 GeV)  but also at low energy.  Almost all collider experiments show difficulties
in the measurement of the diffractive cross section since they do not register
particles emitted into the forward direction.
A new version of the air shower simulation programs AIRES, with an improved treatment
of the diffractive cross section in the low energy hadronic model was developed.
To cross-check this model, we compare the results of the balloon born experiment
CAPRICE98,  on atmospheric fluxes of particles with this new version of AIRES.</abstract>
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