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The Data Processor of the SPB2 Fluorescence Telescope: in flight performance

  • JEM-EUSO Collaboration
  • University of Naples Federico II
  • INFN Sezione di Napoli
  • INFN Sezione di Bari
  • INFN Roma Tor Vergata
  • UTIU
  • Nihon University
  • University of Alabama in Huntsville
  • Astroparticule and Cosmol APC
  • Gran Sasso Science Institute
  • Lehman College
  • INFN Sezione di Catania
  • Istituto di Astrofisica e Planetologia Spaziali (IAPS)
  • INFN Sezione di Torino
  • University of Turin
  • College of Computing
  • Università degli studi di Bari Aldo Moro
  • Moscow State University
  • NASA Marshall Space Flight Center
  • Riken
  • KTH Royal Institute of Technology
  • University of Chicago
  • University of Rome “Tor Vergata”
  • Max-Planck-Institut für Physik
  • Università degli Studi di Catania
  • Joint Laboratory of Optics
  • University of California, Space Sciences Laboratory
  • Pennsylvania State University
  • Science and Research Directorate
  • Colorado School of Mines
  • University of Tokyo
  • Institute of Meteorology and Climate Research
  • Konan University
  • Korea Astronomy and Space Science Institute
  • NASA Goddard Space Flight Center
  • Institute of Physics of the Czech Academy of Sciences
  • National Centre for Nuclear Research
  • University of Utah
  • Univ. Mentouri de Constantine
  • National Astronomical Observatory
  • University of Iowa
  • Joint Institute for Nuclear Research, Dubna
  • Institut Universitaire de France
  • Sungkyunkwan University
  • University of Warsaw
  • LNF-INFN
  • Space Regatta Consortium
  • Hokkaido University
  • Shinshu University
  • University of Geneva
  • Centre de Développement des Technologies Avancées
  • Fairfield University

Research output: Contribution to journalConference articlepeer-review

Abstract

EUSO-SPB2 (Extreme Universe Space Observatory on a Super Pressure Balloon II) is a precursor mission for a future space observatory for multi-messenger astrophysics, planned to be launched in Spring 2023 with a flight duration target of 100 days. The Fluorescence Telescope (FT) hosted on board is designed to detect Ultra High Energy Cosmic Rays via the UV fluorescence emission of the Extensive Air Showers in the atmosphere. The Data Processor (DP) of the FT is the component of the electronics system that performs data management and instrument control for the telescope. The DP controls front-end electronics, tags events with arrival time and payload position through a GPS system, provides signals for time synchronization of the event and measures the live and dead time of the telescope. Furthermore, it manages mass memory for data storage, performs housekeeping monitoring, and controls the power-on and power-off sequences. Finally, the data processor combines the data from the PDMs and onboard differential GPS and prioritizes data for download. The long duration of the flight poses strict requirements on electronics and data handling. The operations at high altitude in an unpressurized environment represent a technological challenge for heat dissipation. This contribution will provide an overview of the innovative elements developed and the results of the integration and field test campaigns. We will also present some preliminary analysis of the performance during the flight.

Original languageEnglish
Article number219
JournalProceedings of Science
Volume444
Publication statusPublished - 27 Sept 2024
Event38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan
Duration: 26 Jul 20233 Aug 2023

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