English

Method of EAS's Cherenkov and fluorescent light separation using silicon photomultipliers

High Energy Astrophysical Phenomena 2019-03-12 v1 Instrumentation and Methods for Astrophysics

Abstract

Preliminary results on the development of a separation method for Cerenkov (CL) and fluorescence (FL) light from EAS are shown. The results are based on the measurement of attenuation coefficients of CL and FL for different filters. A total of six optical filters were investigated: filters from optical glass UFS-1, UFS-5, FS6 (analogue BG3) and interference filters SL 360-50, SL 280-380, FF01-375/110. The measurements were performed using silicon photomultipliers (SiPM). To improve existing fluorescent light detectors, a segment of 7 SiPM was developed, which would be able to separate both components of the light flux from EAS at the level of primary data processing.

Keywords

Cite

@article{arxiv.1811.08851,
  title  = {Method of EAS's Cherenkov and fluorescent light separation using silicon photomultipliers},
  author = {Dmitry Chernov and Elena Bonvech and Timur Dzhatdoev and Miroslav Finger and Michael Finger and Vladimir Galkin and Gali Garipov and Vladimir Kozhin and Dmitry Podgrudkov and Alexander Skurikhin},
  journal= {arXiv preprint arXiv:1811.08851},
  year   = {2019}
}

Comments

6 pages, 5 figures