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SUMMARY:Calculation of radio emission from high energy air showers
DTSTART;VALUE=DATE-TIME:20070706T194500Z
DTEND;VALUE=DATE-TIME:20070706T194500Z
DTSTAMP;VALUE=DATE-TIME:20260417T063643Z
UID:indico-contribution-969@cern.ch
DESCRIPTION:Speakers: Dr. ENGEL\, Ralph (Forschungszentrum Karlsruhe\, Kar
 lsruhe Institute of Technology\, 76021 Karlsruhe)\nFor a long time radio e
 mission accompanying extensive air showers (EAS) is considered\nas an alte
 rnative to traditional methods of high energy cosmic ray detection (> 10^1
 7\neV). In this paper\, results of simulations of radio signals from air s
 howers with\nenergy greater than 10^17 eV are reported. The simulations ar
 e based on a\ntrack-by-track radio emission calculation using the EGSnrc M
 onte Carlo shower code.\nThe lateral distribution of the predicted radio e
 mission pattern is compatible with\nthe recent LOPES-10 experimental data 
 at distances < 300 m. Perspectives of extending\nthe EAS radio emission ca
 lculation to ultra-high energy (up to 10^20 eV) are also\ndiscussed.\n\nht
 tps://indico.nucleares.unam.mx/event/4/session/39/contribution/969
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/39/contribution/969
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