Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/99708
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Type: Journal article
Title: Nanosecond-level time synchronization of autonomous radio detector stations for extensive air showers
Author: Aab, A.
Abreu, P.
Aglietta, M.
Ahn, E.
Al Samarai, I.
Albuquerque, I.
Allekotte, I.
Allison, P.
Almela, A.
Alvarez Castillo, J.
Alvarez-Muñiz, J.
Alves Batista, R.
Ambrosio, M.
Aminaei, A.
Anastasi, G.
Anchordoqui, L.
Andringa, S.
Aramo, C.
Arqueros, F.
Arsene, N.
et al.
Citation: Journal of Instrumentation, 2016; 11(1):P01018-1-P01018-31
Publisher: IOP Publishing
Issue Date: 2016
ISSN: 1748-0221
1748-0221
Statement of
Responsibility: 
The Pierre Auger Collaboration
Abstract: To exploit the full potential of radio measurements of cosmic-ray air showers at MHz frequencies, a detector timing synchronization within 1 ns is needed. Large distributed radio detector arrays such as the Auger Engineering Radio Array (AERA) rely on timing via the Global Positioning System (GPS) for the synchronization of individual detector station clocks. Unfortunately, GPS timing is expected to have an accuracy no better than about 5 ns. In practice, in particular in AERA, the GPS clocks exhibit drifts on the order of tens of ns. We developed a technique to correct for the GPS drifts, and an independent method is used to cross-check that indeed we reach a nanosecond-scale timing accuracy by this correction. First, we operate a “beacon transmitter” which emits defined sine waves detected by AERA antennas recorded within the physics data. The relative phasing of these sine waves can be used to correct for GPS clock drifts. In addition to this, we observe radio pulses emitted by commercial airplanes, the position of which we determine in real time from Automatic Dependent Surveillance Broadcasts intercepted with a software-defined radio. From the known source location and the measured arrival times of the pulses we determine relative timing offsets between radio detector stations. We demonstrate with a combined analysis that the two methods give a consistent timing calibration with an accuracy of 2 ns or better. Consequently, the beacon method alone can be used in the future to continuously determine and correct for GPS clock drifts in each individual event measured by AERA.
Keywords: Pattern recognition; cluster finding; calibration and fitting methods; timing detectors; detector alignment and calibration methods (lasers, sources, particle beams)
Description: Jose A. Bellido Caceres, Simon G. Blaess, Roger W. Clay, Bruce R. Dawson, Trent D. Grubb, Thomas A. Harrison, Maximus D. Malacari, Phong H. Nguyen, Steven J. Saffi, Fred Sarazin, Jennifer S. Sorokin, Patrick van Bodegom, are members of The Pierre Auger collaboration.
Rights: © 2016 IOP Publishing Ltd and Sissa Medialab srl
RMID: 0030043881
DOI: 10.1088/1748-0221/11/01/P01018
Grant ID: http://purl.org/au-research/grants/arc/DP150101622
Appears in Collections:Physics publications

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