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VERSION:2.0
PRODID:-//CERN//INDICO//EN
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SUMMARY:Ultra High Energy Cosmic Rays
DTSTART;VALUE=DATE-TIME:20030507T100000Z
DTEND;VALUE=DATE-TIME:20030507T110000Z
DTSTAMP;VALUE=DATE-TIME:20261112T012424Z
UID:indico-event-1313@indico.ific.uv.es
DESCRIPTION:For ultrahigh energy cosmic rays with energies above 10^18 eV 
 there are still many open questions as "How can particles be accelerated t
 o these energies?" and "What are their sources?". In addition the newest d
 ata from HiRes fluorescence detector\, which seem consistent with a GZK cu
 toff\,show a desagrement with the data from the AGASA ground array. In thi
 s talk I would like to show the results obtained by numerical simulations 
 under different conditions of source distribution\, strenght of extra-gala
 ctic magnetic field and nature of primary particles.\n\nhttps://indico.ifi
 c.uv.es/event/1313/
LOCATION:Edf. Institutos de Investigación Sala Seminarios IFIC
URL:https://indico.ific.uv.es/event/1313/
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