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EUSO-SPB1 mission and science

  • JEM-EUSO
  • Tlemcen University
  • Nihon University
  • University of Alabama in Huntsville
  • Astroparticule and Cosmol APC
  • Universidad Politécnica de Madrid
  • Lehman College
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
  • INFN Sezione di Catania
  • University of Turin
  • INFN Sezione di Torino
  • University of Tokyo
  • Université Badji Mokhtar - Annaba
  • Centre de Développement des Technologies Avancées
  • Universidad de Alcalá
  • Colorado School of Mines
  • College of Computing
  • Institute of Experimental Physics Slovak Academy of Sciences
  • Istituto di Astrofisica e Planetologia Spaziali (IAPS)
  • University of Rome “Tor Vergata”
  • University of Tübingen
  • Instituto Nacional de Técnica Aeroespacial (CSIC/INTA)
  • INFN Sezione di Bari
  • Università degli studi di Bari Aldo Moro
  • Moscow State University
  • NASA Marshall Space Flight Center
  • Institute of Meteorology and Climate Research
  • Riken
  • Centre Suisse d'Electronique et de Microtechnique SA
  • University of Sofia
  • KTH Royal Institute of Technology
  • University of Geneva
  • University of Chicago
  • Universidad Autónoma de Chiapas
  • INFN Sezione di Napoli
  • Max-Planck-Institut für Physik
  • Institute of Space Sciences
  • Università degli Studi di Catania
  • INFN Roma Tor Vergata
  • Joint Laboratory of Optics
  • Kindai University
  • University of Naples Federico II
  • UTIU
  • University of California, Space Sciences Laboratory
  • IRAP/CNRS
  • Astrophysics Division
  • University of León
  • Algiers Observatory
  • LNF-INFN
  • Kyoto University
  • Technical University of Kosice
  • University of Maryland
  • Saitama University
  • Nagoya University
  • Sungkyunkwan University
  • Instituto de Astrofisica de Canarias
  • Konan University
  • National Astronomical Observatory
  • University of M’sila
  • Ulsan National Institute of Science and Technology
  • Korea Astronomy and Space Science Institute
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • NASA Goddard Space Flight Center
  • Biochemical and Environmental Engineering
  • High Energy Accelerator Research Organization (KEK)
  • University of California, Los Angeles
  • Research Unit on Optics and Photonics
  • Institute of Physics of the Czech Academy of Sciences
  • Benemerita Universidad Autonoma de Puebla
  • Chiba University
  • University of Utah
  • Univ. Mentouri de Constantine
  • Universidad Nacional Autónoma de México
  • University of Iowa
  • Osaka City University
  • ETH Zurich
  • University of Warsaw
  • Space Regatta Consortium
  • Hokkaido University
  • ISAS/JAXA
  • Osaka Electro-Communication University
  • Centro Mesoamericano de Física Teórica (MCTP)
  • Joint Institute for Nuclear Research, Dubna
  • Shinshu University
  • National Institutes for Quantum and Radiological Science and Technology
  • Universidad Michoacana de San Nicolás de Hidalgo
  • Kanazawa University

Research output: Contribution to journalArticlepeer-review

34 Citations (Scopus)

Abstract

The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. The plan of this mission of opportunity on a NASA super pressure balloon test flight was to circle the southern hemisphere. The primary scientific goal was to make the first observations of ultra-high-energy cosmic-ray extensive air showers (EASs) by looking down on the atmosphere with an ultraviolet (UV) fluorescence telescope from suborbital altitude (33 km). After 12 days and 4 h aloft, the flight was terminated prematurely in the Pacific Ocean. Before the flight, the instrument was tested extensively in the West Desert of Utah, USA, with UV point sources and lasers. The test results indicated that the instrument had sensitivity to EASs of ⪆3 EeV. Simulations of the telescope system, telescope on time, and realized flight trajectory predicted an observation of about 1 event assuming clear sky conditions. The effects of high clouds were estimated to reduce this value by approximately a factor of 2. A manual search and a machine-learning-based search did not find any EAS signals in these data. Here we review the EUSO-SPB1 instrument and flight and the EAS search.

Original languageEnglish
Article number102891
JournalAstroparticle Physics
Volume154
DOIs
Publication statusPublished - 1 Jan 2024

Keywords

  • Air fluorescence
  • Cosmic rays (329)
  • Extensive air showers
  • High-altitude balloons (738)
  • JEM-EUSO

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