Timing calibration and directional reconstruction for Tunka-HiSCORE

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Abstract

The Tunka-HiSCORE detector follows the concept of a non-imaging wide-angle EAS Cherenkov array, designed to search for γ-ray sources above 10 TeV and to investigate the spectrum and composition of cosmic-rays above 100 TeV. A prototype array with 9 stations has been deployed in October 2013 at the site of the Tunka experiment in Russia. We describe design and performance of the array data acquisition system DAQ-2, focusing on its timing system based on the White Rabbit technology for sub-nsec time-synchronization over ethernet. First results of EAS arrival direction reconstruction, compared with MC simulations, and tests with artifical light sources verify an excellent performance of the system.

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Porelli, A., Bogorodskii, D., Brückner, M., Budnev, N., Chvalaev, O., Dyachok, A., … Zurbanov, V. (2015). Timing calibration and directional reconstruction for Tunka-HiSCORE. In Journal of Physics: Conference Series (Vol. 632). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/632/1/012041

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