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The JEM-EUSO MissionJEM-EUSO is a science mission to explore extremes of the Universe. It observes the dark-side of the Earth and detects UV photons emitted from the extensive air shower caused by an extreme energy particle (about 10(exp 20) eV). Such a particle arrives almost straightly through our Milky Way Galaxy and is expected to allow us to trace the source location by its arrival direction. This will open the door to the new astronomy with charged particles. In its five years operation including the tilted mode, JEM-EUSO will detect at least 1,000 events with E>7 X 10(exp 19) eV and determine the energy spectrum of trans-GZK region with a statistical accuracy of several percent. JEM-EUSO is planned to be transported with HTV (H2 Transfer Vehicle) and attached to the Japanese Experiment Module/ Exposure Facility (JEM/EF) of International Space Station. JAXA has selected JEM-EUSO for one of the mission candidates of the second phase utilization of JEM/EF for the launch of early 2010s. One year-long phase-A study will be carried out under JAXA.
Document ID
20090028813
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Adams, J.H.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Christl, M.J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Watts, J.W.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 24, 2013
Publication Date
July 3, 2007
Subject Category
Astronomy
Report/Patent Number
MSFC-314
Report Number: MSFC-314
Meeting Information
Meeting: 30th International Cosmic Ray Conference
Location: Merida, Yucatan
Country: Mexico
Start Date: July 3, 2007
End Date: July 11, 2007
Sponsors: International Union of Pure and Applied Physics
Distribution Limits
Public
Copyright
Public Use Permitted.
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