Paper
28 December 2007 FPGA based triggers in the Pierre Auger Observatory
Z. Szadkowski
Author Affiliations +
Proceedings Volume 6937, Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2007; 69370U (2007) https://doi.org/10.1117/12.784612
Event: Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2007, 2007, Wilga, Poland
Abstract
The Pierre Auger Observatory is an international project for research on ultra-high energy cosmic rays (UHECR) above 1019 eV and currently the world largest "hybrid" experiment. The hybrid technique uses both the detection of particles at the ground in water Cherenkov detectors (WCD) and measurements of fluorescence light generated in the atmosphere by the extensive air showers. This technique offers unique possibilities for cross-calibration and reduction of measurement uncertainties. The surface array will contain 1600 surface detector stations distributed over 3000 km2 in the Southern Hemisphere (under construction in Argentina) and 4000 WCD distributed over 10000 km2 at a Northern Hemisphere site in Colorado (deployment planned for 2008). Four fluorescence stations each containing 6 wide-angle Schmidt telescopes and each equipped with 440 PMTs with 1.5° angle resolution and 30 • 30° of field of view are located on the border of the surface array in the Southern Site. The paper presents implementations of the FPGA used for triggering. The use is illustrated with currently working schemes as well as other possible ideas especially promising for the surface detector in which currently used triggers seems to be not effective enough for very inclined and horizontal showers. Proposed new triggers enlarge a simple 1-bit threshold detection to the online analysis of a FADC trace shape. This corresponds to a charge from PMTs or signal power estimation. The next category is spectral triggers analyzing sequential samples in the frequency domain. Digital sigma-delta filters immunize the trigger circuitry on the pedestal variation as results of huge temperature swings. Presented DCT trigger provides native pedestal independence.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Z. Szadkowski "FPGA based triggers in the Pierre Auger Observatory", Proc. SPIE 6937, Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2007, 69370U (28 December 2007); https://doi.org/10.1117/12.784612
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KEYWORDS
Sensors

Field programmable gate arrays

Clocks

Digital signal processing

Luminescence

Muons

Observatories

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