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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>
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<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>
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  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <title>The Northern Site of The Pierre Auger Observatory</title>
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   <title>Prof.</title>
   <name first="David" middle="" last="Nitz"></name>
   <organization>Michigan Technological University</organization>
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   <organization>Pierre Auger Observatory</organization>
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   <title>Prof.</title>
   <name first="David" middle="" last="Nitz"></name>
   <organization>Michigan Technological University</organization>
   <emailHash>51ac3912dee0e53ff37ad86f3ff56713</emailHash>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Yucatan II+III+IV (Fiesta Americana)</room>
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 <startDate>2007-07-10T11:42:00</startDate>
 <endDate>2007-07-10T11:54:00</endDate>
 <duration>00:12</duration>
 <abstract>The Pierre Auger Observatory is a multi-national project for research on ultra-high
energy cosmic rays.  The Southern Auger Observatory in Mendoza province, Argentina,
is approaching completion in 2007 with an instrumented area of 3,000 square
kilometers.  It will accurately measure the spectrum and composition of ultra-high
energy cosmic rays up to and beyond the predicted GZK feature.  We have obtained
first results on the energy spectrum, mass composition and distribution of arrival
directions on the southern sky.

The Northern Auger Observatory is designed to complete and extend the investigations
begun in the south. It will establish charged particle astronomy and thus open a new
window into the universe. The distribution of arrival directions of the highest
energy events will point the way to unveiling the almost century old mystery of the
origin and nature of ultra-high energy cosmic rays.  Achieving this goal requires
collecting many more events in spite of the steeply falling energy spectrum. The
planned northern site will have an instrumented area of 4,000 square miles (10,370
square kilometers) in South-East Colorado, USA. The presentation covers the science
of particle astronomy, the layout and the technical implementation of the Northern
Auger Observatory.</abstract>
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