Trigger developments for the fluorescence detector of EUSO-TA and EUSO-SPB2
M. Battisti, M. Bertaina, F. Fenu, H. Miyamoto, K. Shinozaki, A., Belov, F. Bisconti, M. Mignone, F. Capel (for the JEM-EUSO Collaboration)

TL;DR
This paper discusses the development of a multi-scale trigger system for the fluorescence detectors of EUSO-TA and EUSO-SPB2, enhancing detection capabilities for cosmic rays and other atmospheric events.
Contribution
It introduces a new trigger logic tailored for different detector configurations, building upon previous designs for Mini-EUSO, with dynamic thresholding and event detection on multiple time scales.
Findings
Development of L1 trigger logic for EUSO-TA and EUSO-SPB2
Implementation of dynamic pixel thresholding
Testing of trigger logic performance
Abstract
The JEM-EUSO program aims at detecting Ultra High Energy Cosmic Rays (UHECRs) by observing the fluorescence light produced by extensive air showers (EAS) in the Earth's atmosphere. Within this program, a new generation of missions is being built, including (i) Mini-EUSO that will be installed on board the ISS in August 2019, (ii) an upgrade to the ground-based telescope EUSO-TA and (iii) the second super pressure balloon flight (EUSO-SPB2). All these detectors will have a dedicated trigger system based on a board equipped with a Xilinx Zynq device that will be able to detect different types of events on three different time-scales: a microsecond time-scale for cosmic ray detection (L1), a hundreds of microsecond time-scale for slower events like transient luminous events (TLEs) (L2), and a tens of millisecond time-scale used to produce a continuous monitoring, for even slower events…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Particle Detector Development and Performance
