DocumentCode :
1521938
Title :
Triggers, Data Flow and the Synchronization Between the Auger Surface Detector and the AMIGA Underground Muon Counters
Author :
Szadkowski, Zbigniew
Author_Institution :
Dept. of Phys. & Appl. Inf., Univ. of Lodz, Lodz, Poland
Volume :
58
Issue :
4
fYear :
2011
Firstpage :
1771
Lastpage :
1777
Abstract :
The aim of the AMIGA project (Auger Muons and Infill for the Ground Array) is an investigation of Extensive Air Showers at energies lower than those accesible with the standard Auger array, where the transition from galactic to extragalactic sources is expected. The paper describes the working principle of the Master/Slave (standard Auger surface detector/the underground muon counters) synchronous data acquisition and general triggering applied in two prototypes: with 12.5 ns resolution built from 4 segments (2 FPGAs and 2 standard micro-controllers) and 3.125 ns resolution built from two segments only (2 FPGAs with implemented NIOS® processors).
Keywords :
Cherenkov counters; cosmic ray apparatus; cosmic ray muons; cosmic ray origin; cosmic ray showers; data acquisition; field programmable gate arrays; microcontrollers; nuclear electronics; scintillation counters; AMIGA project; AMIGA underground muon counters; Auger Muons and Infill for the Ground Array; Auger surface detector; FPGA; NIOS processors; cosmic ray extragalactic sources; cosmic ray galactic sources; detector data flow; detector synchronization; detector trigger; extensive air showers; master-slave synchronous data acquisition; microcontrollers; Detectors; Field programmable gate arrays; Mesons; Prototypes; Radiation detectors; Random access memory; Synchronization; FPGA; NIOS; Pierre Auger observatory; trigger;
fLanguage :
English
Journal_Title :
Nuclear Science, IEEE Transactions on
Publisher :
ieee
ISSN :
0018-9499
Type :
jour
DOI :
10.1109/TNS.2011.2142194
Filename :
5771580
Link To Document :
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