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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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 <name>Merida, Mexico</name>
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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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 <board>149 (8A)</board>
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 <title>In-orbit counting rates measured by the PAMELA anticoincidence system</title>
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   <name first="Silvio" middle="" last="Orsi"></name>
   <organization>Royal Institute of Technology</organization>
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   <organization>Royal Institute of Technology</organization>
   <emailHash>4cc56a8e3cf2b710fd854e654b099797</emailHash>
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   <organization>Royal Institute of Technology</organization>
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   <organization>Royal Institute of Technology</organization>
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   <name first="Petter" middle="" last="Hofverberg"></name>
   <organization>Royal Institute of Technology</organization>
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   <name first="Mark" middle="" last="Pearce"></name>
   <organization>Royal Institute of Technology</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
 </location>
 <startDate>2007-07-04T14:45:00</startDate>
 <endDate>2007-07-04T14:45:00</endDate>
 <abstract>PAMELA is a satellite-borne experiment designed to study the charged component of the
cosmic radiation of galactic, solar and trapped nature. The main scientific objective
is the study of the antimatter component of cosmic rays over a wide range of
energies. PAMELA is mounted on the Resurs DK1 satellite that was launched on June
15th 2006 from the Baikonur cosmodrome and is now on a semipolar (70°) elliptical
(350×600 km^2) orbit. The PAMELA apparatus consists of a permanent magnet silicon
spectrometer, an electromagnetic imaging calorimeter, a time of flight system, a
scintillator-based anticoincidence (AC) system, a tail
catcher scintillator and a neutron detector. The AC system can be used to reject
particles not cleanly entering the PAMELA acceptance. A standalone study of the
functionality of the AC system during in-flight operations is presented. The in-orbit
particle rates measured by the AC system during the first 6 months of operation are
shown. The orbital dependence of the particle rates, the energy and the
directionality of the trapped particles are also discussed.</abstract>
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