3-11 July 2007
Merida, Mexico
Mexico/General timezone
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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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Displaying 2 contributions out of 2
Type: Oral Session: HE 1.2.B
Track: HE.1.2.B
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
Type: Oral Session: HE 1.2.B
Track: HE.1.2.B
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
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