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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>Galactic Cosmic Ray Modulation in the Heliosphere at Solar Maximum</title>
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   <name first="Oscar G." middle="" last="Morales-Olivares"></name>
   <organization>IPN, ESIA</organization>
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   <title></title>
   <name first="Oscar G." middle="" last="Morales-Olivares"></name>
   <organization>IPN, ESIA</organization>
   <emailHash>fa66977fad9798c9c848cdd9ef3eb439</emailHash>
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   <title>Dr.</title>
   <name first="Rogelio A." middle="" last="Caballero-Lopez"></name>
   <organization>UNAM, Institute of Geophysics</organization>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
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 <startDate>2007-07-09T14:45:00</startDate>
 <endDate>2007-07-09T14:45:00</endDate>
 <abstract>The spatial distribution of galactic cosmic rays in the heliosphere 
at solar maximum of Cycles  21, 22 and 23 are studied using a one 
dimensional model of the cosmic ray transport equation. We investigated 
the radial intensity gradients from 1 AU to the distant heliosphere and 
interpreted the data from IMP8, Voyagers 1/2, Pioneer 10 and balloon 
experiment BESS. In our model we considered three of the physical processes 
that affect the cosmic radiation: diffusion, convection and adiabatic 
energy loss. Our analysis indicates that adiabatic energy loss plays an 
important role in the radial distribution of galactic cosmic ray in the 
inner heliosphere, while in the outer region the diffusion and convection 
are the relevant processes.</abstract>
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