Published 2019 | Version v1
Book

Results from the first missions of the JEM-EUSO program

  • 1. National Institute for Nuclear Physics - INFN-Turin, Turin (Italy)
  • 2. Department of Physics, University of Turin, Turin (Italy)

Description

The origin and nature of Ultra-High Energy Cosmic Rays (UHECRs) remain unsolved in contemporary astro particle physics. To give an answer to these questions is rather challenging because of the extremely low flux of a few per km2 per century at extreme energies such as E > 5*1019 eV. The objective of the JEM-EUSO program, Extreme Universe Space Observatory, is the realization of a space mission devoted to scientific research of cosmic rays of highest energies. Its super-wide-field telescope will look down from space onto the night sky to detect UV photons emitted from air showers generated by UHECRs in the atmosphere. The JEM-EUSO program includes different missions using fluorescence detectors to make a proof-of-principle of the UHECR observation from space and to raise the technological level of the instrumentation to be employed in a space mission. EUSO-TA, installed at the Telescope Array site in Utah in 2013, is in operation. It has already detected 9 UHECRs in coincidence with Telescope Array fluorescence detector at Black Rock Mesa. EUSO-Balloon flew on board a stratospheric balloon in August 2014. It measured the UV intensity on forests, lakes and the city of Timmins as well as proved the observation of UHECR-like events by shooting laser tracks. EUSO-SPB was launched on board a super pressure balloon on April 25. and flew for 12 days. It proved the functionality of all the subsystems of the telescope on a typical duration of a balloon flight; observed the UV emission on oceans and has a self-trigger system to observe UHECRs with energy E > 3*1018 eV. TUS, the Russian mission on board the Lomonosov satellite in orbit since April 28. 2016, is now included in the JEM-EUSO program and has detected so far in the UHECR trigger-mode a few interesting signals. Mini-EUSO is in its final phase of integration in Italy, where several performance tests are being held. Mini-EUSO will be installed inside the International Space Station (ISS) in 2019. The main results obtained so far by such missions are summarized and put in prospect of future space detectors such as K-EUSO and POEMMA. (authors)

Availability note (English)

Available from doi: http://dx.doi.org/10.1051/epjconf/201921005009
Part of:
EPJ Web of Conferences, Proceedings of the 2018 International Symposium on Ultra-High-Energy Cosmic Rays - UHECR-2018

Additional details

Identifiers

Publishing Information

Publisher
EDP Sciences
Imprint Place
Les Ulis (France)
Imprint Title
EPJ Web of Conferences, Proceedings of the 2018 International Symposium on Ultra-High-Energy Cosmic Rays - UHECR-2018
Imprint Pagination
v. 210 [408 p.]
Journal Page Range
p. 05009.p.1-05009.p.6

Conference

Title
UHECR-2018 - 2018 International Symposium on Ultra-High-Energy Cosmic Rays
Dates
8-12 Oct 2018
Place
Paris (France)

INIS

Country of Publication
France
Country of Input or Organization
France
INIS RN
50058762
Subject category
S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COSMIC RAY DETECTION; DATA ANALYSIS; EEV RANGE; RADIATION DETECTORS; TELESCOPE COUNTERS
Descriptors DEC
DATA PROCESSING; DETECTION; ENERGY RANGE; MEASURING INSTRUMENTS; PROCESSING; RADIATION DETECTION

Optional Information

Notes
22 refs.
Collaborations
JEM-EUSO Collaboration