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The EUSO-Balloon pathfinder

  • The JEM-EUSO Collaboration
  • University of Alabama in Huntsville
  • Université Paris-Sud
  • Laboratoire de l'Accélérateur Linéaire
  • Laboratoire de Probabilités et Modèles Aléatoires
  • University of Wisconsin-Milwaukee
  • University of California, Los Angeles
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
  • INFN Sezione di Catania
  • High Energy Accelerator Research Organization (KEK)
  • Interactive Research Center of Science
  • Tokyo Institute of Technology
  • Universidad de Alcalá
  • Dipartimento di Ingegneria
  • UTIU
  • Astrophysics Division
  • University of Tübingen
  • Dipartimento di Fisica
  • University of Turin
  • Instituto Nacional de Técnica Aeroespacial (CSIC/INTA)
  • INFN
  • INFN Sezione di Bari
  • Universita’ degli Studi di Bari Aldo Moro and INFN
  • Università degli studi di Bari Aldo Moro
  • Vanderbilt University
  • INFN Sezione di Torino
  • Institute of Meteorology and Climate Research
  • Joint Institute for Nuclear Research, Dubna
  • Centre Suisse d'Electronique et de Microtechnique SA
  • Polish Academy of Sciences
  • Department of Space Physics
  • Institute of Experimental Physics Slovak Academy of Sciences
  • University of Sofia
  • Universidad Carlos III de Madrid
  • INFN Sezione di Napoli
  • Department of Physics and Astronomy
  • Università degli Studi di Catania
  • INFN Roma Tor Vergata
  • Riken
  • Istituto Di Fisica Applicata Nello Carrara
  • IRAP/CNRS
  • Istituto di Astrofisica e Planetologia Spaziali (IAPS)
  • Kindai University
  • NASA Marshall Space Flight Center
  • Universidad Nacional Autónoma de México

Research output: Contribution to journalArticlepeer-review

42 Citations (Scopus)

Abstract

EUSO-Balloon is a pathfinder for JEM-EUSO, the Extreme Universe Space Observatory which is to be hosted on-board the International Space Station. As JEM-EUSO is designed to observe Ultra-High Energy Cosmic Rays (UHECR)-induced Extensive Air Showers (EAS) by detecting their ultraviolet light tracks “from above”, EUSO-Balloon is a nadir-pointing UV telescope too. With its Fresnel Optics and Photo-Detector Module, the instrument monitors a 50 km2 ground surface area in a wavelength band of 290–430 nm, collecting series of images at a rate of 400,000 frames/sec. The objectives of the balloon demonstrator are threefold: a) perform a full end-to-end test of a JEM-EUSO prototype consisting of all the main subsystems of the space experiment, b) measure the effective terrestrial UV background, with a spatial and temporal resolution relevant for JEM-EUSO. c) detect tracks of ultraviolet light from near space for the first time. The latter is a milestone in the development of UHECR science, paving the way for any future space-based UHECR observatory. On August 25, 2014, EUSO-Balloon was launched from Timmins Stratospheric Balloon Base (Ontario, Canada) by the balloon division of the French Space Agency CNES. From a float altitude of 38 km, the instrument operated during the entire astronomical night, observing UV-light from a variety of ground-covers and from hundreds of simulated EASs, produced by flashers and a laser during a two-hour helicopter under-flight.

Original languageEnglish
Pages (from-to)281-299
Number of pages19
JournalExperimental Astronomy
Volume40
Issue number1
DOIs
Publication statusPublished - 1 Nov 2015
Externally publishedYes

Keywords

  • Air-fluorescence
  • Balloon experiment
  • JEM-EUSO
  • UHECR

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