3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
HE 1.2.B
Place
Location: Merida, Mexico
Room: Yucatan II+III+IV (Fiesta Americana)
Date:
9 Jul 11:10 - 11:34
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The radio emission from cosmic ray air showers consists in large part of
geosynchrotron radiation. Since the radiation mechanism is based on
particle acceleration, atmospheric electric fields may play an important
role. LOPES results show that electric fields under fair weather conditions
do not alter the radio emission considerably, but during thunderstorms
strongly amplified pulses are meas
... More
Presented by Mr. Stijn BUITINK
on
9/7/2007
at
16:10
With full coverage and high observation altitude, the ARGO-YBJ experiment
offer us an opportunity to get further information for the cosmic ray spectrum
in the 'knee region' and the spectrum from different primaries.
On the base of Monte Carlo Simulation, a large simulation sample are generated.
Several parameters are introduced which describe the shower lateral
distribution, front plane and
... More
Presented by Mr. song zhan CHEN