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  <organization>ICN-UNAM</organization>
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  <userid>3</userid>
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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>
<participants></participants>
<closed>True</closed>
<location>
 <name>Merida, Mexico</name>
 <address></address>
 <room></room>
</location>
<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>
<chair>
 <user>
  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
 </user>
</chair>
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 <board>050 (3A)</board>
 <track>HE.1.5</track>
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  <name>Poster</name>
 </type>
 <title>Atmospheric Monitoring System of the JEM-EUSO Mission</title>
 <speakers>
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   <title>Dr.</title>
   <name first="Valentin" middle="" last="Mitev"></name>
   <organization>Observatory of Neuchâtel,  Switzerland</organization>
   <emailHash>a4ab141d30eccdab472084496330c2af</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Mitsuteru" middle="" last="Sato"></name>
   <organization>RIKEN, Japan</organization>
   <emailHash>a49c73ce1cbc7a417eab38638f8ffb10</emailHash>
  </user>
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   <title>Dr.</title>
   <name first="Valentin" middle="" last="Mitev"></name>
   <organization>Observatory of Neuchâtel,  Switzerland</organization>
   <emailHash>a4ab141d30eccdab472084496330c2af</emailHash>
  </user>
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   <title>Dr.</title>
   <name first="Mitsuteru" middle="" last="Sato"></name>
   <organization>RIKEN, Japan</organization>
   <emailHash>a49c73ce1cbc7a417eab38638f8ffb10</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Toshikazu" middle="" last="Ebisuzaki"></name>
   <organization>RIKEN, Japan</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Y." middle="" last="Takizawa"></name>
   <organization>RIKEN, Japan</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Y." middle="" last="Kawasaki"></name>
   <organization>RIKEN, Japan</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Renaud" middle="" last="Matthey"></name>
   <organization>Observatory of Neuchâtel, Switzerland</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
 </coAuthors>
 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
 </location>
 <startDate>2007-07-06T14:45:00</startDate>
 <endDate>2007-07-06T14:45:00</endDate>
 <abstract>JEM-EUSO will study ultra-high-energy cosmic rays by their optical yield in the 
atmosphere. To evaluate this yield it is important to monitor the atmosphere 
inside the field-of-view (FOV) of the JEM-EUSO receiver. This monitoring shall 
permit the correction of the JEM-EUSO signal, where the critical parameters are 
the cloud presence and top altitude. The Atmospheric Monitoring System will be 
based on a complex of sensors: infrared (IR) camera, Lidar, and JEM-
EUSO "slow-data". The IR camera consists of Ge dioptric lenses, a band-pass 
filter and an un-cooled micro-bolometer array. It will acquire images of the cloud 
top temperature covering the JEM-EUSO FOV. The cloud-top altitude will be 
evaluated from the temperature with relatively low precision. High-precision 
(30m) Lidar cloud-top altitude measurements will be used to correct the cloud-
top altitude from the IR-camera. The Lidar will use laser at 355nm transmitted in 
three fixed directions, as well as the JEM-EUSO receiver with 
three dedicated detector. The optical background signal in the UV, detected by 
JEM-EUSO will allow imaging of the cloud field inside its FOV (the JEM-
EUSO "slow-data" operation). The "stereoscope" processing of this image will 
provide additional low-resolution evaluation of the cloud top altitude.</abstract>
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