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arxiv: 1811.08851 · v1 · pith:T2MBS7P6new · submitted 2018-11-21 · 🌌 astro-ph.HE · astro-ph.IM

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

classification 🌌 astro-ph.HE astro-ph.IM
keywords filterslightfluorescentmethodopticalphotomultipliersresultsseparation
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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.

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