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<supportEmail caption="Support">icrc2007@icrc2007.unam.mx</supportEmail>
<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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<closed>True</closed>
<location>
 <name>Merida, Mexico</name>
 <address></address>
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<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
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 <title>The JEM-EUSO Mission</title>
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   <organization>RIKEN</organization>
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   <emailHash>086722ca93eefe3a2f83da6cef6f2730</emailHash>
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   <name first="Y." middle="" last="Takahashi"></name>
   <organization>RIKEN, Japan and UAH, USA</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
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   <name first="F." middle="" last="Kajino"></name>
   <organization>Konan Univ., Japan</organization>
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   <organization>Saitama Univ., Japan</organization>
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   <organization>RIKEN, Japan</organization>
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   <organization>Univ. of Torino, Italy</organization>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Yucatan II+III+IV (Fiesta Americana)</room>
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 <startDate>2007-07-10T08:42:00</startDate>
 <endDate>2007-07-10T08:54:00</endDate>
 <duration>00:12</duration>
 <abstract>JEM-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 giant air shower caused by an extremely high energy particle (about
10^20 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: JEM-EUSO can determine the arrival direction of the
particles within several degrees and energy of them within 30%. In its
five years operation including the tilt mode, JEM-EUSO will detect at
least 1,000 events with E&gt;7x10^19 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 released the call for proposals for
the mission candidates of the second phase utilization of JEM/EF for the
launch of 2011 and 2013. Two years of phase-A study will be carried out
under JAXA for selected candidates.
*the JEM-EUSO Collaboration: the list of authors is attached.</abstract>
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