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<category>Conferences</category>
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<announcer>
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  <title></title>
  <name first="Admin" middle="" last="Indico"></name>
  <organization>ICN-UNAM</organization>
  <emailHash>1482bc95ee34f0461176da21871284c8</emailHash>
  <userid>3</userid>
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</announcer>
<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>
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</chair>
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 <board>072 (4A)</board>
 <track>HE.1.5</track>
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  <name>Poster</name>
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 <title>The TALE Tower Detector</title>
 <speakers>
  <user>
   <title>Prof.</title>
   <name first="Douglas" middle="" last="Bergman"></name>
   <organization>Rutgers University</organization>
   <emailHash>ab4590e55f2195397ed8782191e6ba1f</emailHash>
  </user>
 </speakers>
 <primaryAuthors>
  <user>
   <title>Prof.</title>
   <name first="Douglas" middle="" last="Bergman"></name>
   <organization>Rutgers University</organization>
   <emailHash>ab4590e55f2195397ed8782191e6ba1f</emailHash>
  </user>
 </primaryAuthors>
 <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>The TA Low Energy Extension will include a Tower FluorescenceDetector.  Extensive air
showers at the lowest usful energies for fluorescence detectors will in general be
close to the detector.  This requires viewing all elevation angles to be able to
reconstruct showers.  The TALE Tower Detector, operating in conjunction with other
TALE detectors will view elevation angles up to above 70 degrees, with an azimuthal
coverage of about 90 degrees.  Results from a prototype mirror operated in
conjunction with the HiRes detector will also be presented.</abstract>
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