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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>
<participants></participants>
<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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</chair>
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 <board>177 (9A)</board>
 <track>SH.3.1</track>
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 <title>Modeling of the heliospheric structure and cosmic rays inside</title>
 <speakers>
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   <title>Dr.</title>
   <name first="Stefan" middle="" last="Ferreira"></name>
   <organization>North-West University (Potchefstroom Campus)</organization>
   <emailHash>e1e4f804609c14be948daa33ac9520bb</emailHash>
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   <name first="Jasper" middle="" last="Snyman"></name>
   <organization>North-West University (Potchefstroom Campus)</organization>
   <emailHash>e1e4f804609c14be948daa33ac9520bb</emailHash>
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   <title>Dr.</title>
   <name first="Stefan" middle="" last="Ferreira"></name>
   <organization>North-West University (Potchefstroom Campus)</organization>
   <emailHash>e1e4f804609c14be948daa33ac9520bb</emailHash>
  </user>
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   <title>Prof.</title>
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   <organization>North-West University (Potchefstroom Campus)</organization>
   <emailHash>18f2f291e3cb20b819287892ed241e54</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Klaus" middle="" last="Scherer"></name>
   <organization>Ruhr-Universität Bochum</organization>
   <emailHash>b52832eb252baa1e9236bb488bbb9e4a</emailHash>
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 <location>
  <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>The heliospheric interface is calculated using a three-fluid hydrodynamic model. 
Using this approach the effects of different solar wind profiles, as they may 
occur during different levels of solar activity, on the heliospheric structure and 
the distribution of hydrogen and pickup ions are calculated self-consistently. 
We present a time dependent parameter study with respect to the solar wind 
density, velocity, and temperature varying over a solar cycle and its influence 
onto the heliospheric structure and the distribution of anomalous and galactic 
cosmic rays.</abstract>
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