Passer à la navigation principale Passer à la recherche Passer au contenu principal

EUSO-SPB1 mission and science

  • JEM-EUSO
  • Telecom Lab.
  • 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
  • Institute for Cosmic Ray Research
  • University of Tokyo
  • LPR at Department of Physics
  • 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”
  • Institute for Astronomy and Astrophysics
  • 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

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

34 Citations (Scopus)

Résumé

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.

langue originaleAnglais
Numéro d'article102891
journalAstroparticle Physics
Volume154
Les DOIs
étatPublié - 1 janv. 2024

Empreinte digitale

Examiner les sujets de recherche de « EUSO-SPB1 mission and science ». Ensemble, ils forment une empreinte digitale unique.

Contient cette citation