Abstract—
A technique is proposed for carrying out flight calibration of a photomultiplier tubes (PMTs) of the photodetector in the orbital TUS detector of ultra-high-energy cosmic rays in the absence of a calibration signal. The new technique consists in calculating two statistical characteristics of digitized signals from detected events (their mean value A and variance \(\sigma _{A}^{2}\)) and constructing the linear approximation \(\sigma _{A}^{2}\)(A) for stationary signals. This technique has been tested in a laboratory experiment with a photodetector module, which is identical to the modules used in the detector. As a result, the gains of most photodetector channels of the TUS detector have been estimated again and the changes that occurred (in particular, the “aging effect”) have been analyzed.
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Notes
We will use index f (fluctuation) to distinguish the gain obtained in this way from the direct calibration (1).
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This work was supported by the State Corporation Roscosmos and the Fundamental and Applied Space Research Interdisciplinary Scientific and Educational School of the Moscow State University.
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Translated by N. Goryacheva
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Klimov, P.A., Sigaeva, K.F. & Sharakin, S.A. Flight Calibration of the Photodetector in the TUS Detector. Instrum Exp Tech 64, 450–455 (2021). https://doi.org/10.1134/S0020441221030192
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DOI: https://doi.org/10.1134/S0020441221030192