  The origin of Ultra-High Energy Cosmic Rays (UHECRs) remains unsolved in
contemporary astroparticle physics. The objective of the JEM-EUSO program is
the realization of a space mission devoted to UHECR physics. Several detectors
have been developed in this framework or are under development. EUSO-TA,
installed at the Telescope Array site in Utah in 2013, is in operation. It has
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 cities as well as
proved the observation of UHECR-like events reproduced by laser tracks.
EUSO-SPB1 was launched on board a super pressure balloon on April 24th 2017 and
flew for 12 days. It proved the functionality of all the subsystems of the
telescope on a long term and observed the UV emission on oceans. TUS, on board
the Lomonosov satellite, in orbit since April 28th 2016, is now included in he
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 Russia,
and is scheduled for launch on August 22$^{nd}$. The main results obtained so
far by these missions are summarized and put in the perspective of future space
detectors such as K-EUSO and POEMMA.
