The origin and nature of Ultra-High Energy Cosmic Rays (UHECRs) remain unsolved in contemporary astroparticle physics. A cutoff in the cosmic ray energy spectrum clearly appears at ∼ 1020 eV in the data of HIRES, Telescope Array and Auger on ground experiments. It is well known that the detection of events with energy ≥ 1020eV is challenged by the GZK effect, which limits the highest detectable energy at ∼ 1020 eV due to photopion production in the interaction of UHECR on the microwave fossil radiation of the Big Bang, as suggested also by the HIRES and Telescope Array data, or by nuclei photodisintegration as indicated by the Auger results. However, the possibility that the cutoff at ∼ 1020eV can be intrinsic to the acceleration power of the astrophysics cosmic ray sources remains alive. Moreover, indications of sources or excesses in the arrival direction distribution of UHECRs have been claimed by Telescope Array, in the Northern Hemisphere, and by Auger, in the Southern Hemisphere. 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 × 1019eV.
The objective of the JEM-EUSO program, Joint Experiment Missions for 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.
More than 250 researchers from 16 countries are collaborating in JEM-EUSO, with the support of the most important International and National Space Agencies and research funding institutions.
June 15 - 19, 2020 @SINP, MSU, Moscow, Russia
December 2 - 6, 2019 @RIKEN, Wako, Japan
June 10 - 14, 2019 @Lodz, Poland
December 3 - 7, 2018 @Kobe, Hyogo, Japan
The 23rd JEM-EUSO International Collaboration Meeting
June 11 - 15, 2018 @Mürren, Switzerland
December 4 - 8, 2017 @RIKEN, Wako, Japan
July 12 - 20, 2017 @Busan, South Korea
The 21st JEM-EUSO International Collaboration Meeting
June 19 - 24, 2017 @University of Chicago, Chicago, USA
The 20th JEM-EUSO International Collaboration Meeting
December 12 - 16, 2016 @RIKEN, Wako, Japan
The 19th JEM-EUSO International Collaboration Meeting
June 20 - 24, 2016 @APC, Paris, France
The 18th JEM-EUSO International Collaboration Meeting
December 7 - 11, 2015 @Stockholm, Sweden
The 34th International Cosmic Ray Conference (ICRC2015)
July 30 - August 6, 2015 @Hague, The Netherlands
The 17th JEM-EUSO International Collaboration Meeting
June 22 - 26, 2015 @RIKEN, Wako, Japan
Launched on Soyuz MS-13 on August 22nd, 2019. Soyuz successfully docked to ISS on August 26th. First light was observed on October 7th(UTC). Many ELVES and meteors have been detected in several observation sessions.
Conceptual design stage has ended in 2019.
Launched in August 2014. Data analysis in progress.
Launched in April 2017. Data analysis in progress.
Launch is planned in 2022. Design and fabrication in progress.
Upgrade of the DAQ electronics is planned in 2019/2020. Data analysis in progress.