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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>
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<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>
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  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <title>New approach to UHE cosmic ray investigations in the energy range 10^15 - 10^19 eV</title>
 <speakers>
  <user>
   <title>Dr.</title>
   <name first="Igor" middle="" last="Yashin"></name>
   <organization>Moscow Engineering Physics Institute (State University)</organization>
   <emailHash>0b2613e50006e0ee52ab963927f24a84</emailHash>
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  <user>
   <title>Dr.</title>
   <name first="Igor" middle="" last="Yashin"></name>
   <organization>Moscow Engineering Physics Institute (State University)</organization>
   <emailHash>0b2613e50006e0ee52ab963927f24a84</emailHash>
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 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Yucatan II+III+IV (Fiesta Americana)</room>
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 <startDate>2007-07-06T10:42:00</startDate>
 <endDate>2007-07-06T10:54:00</endDate>
 <duration>00:12</duration>
 <abstract>A new approach to investigations of ultra-high energy cosmic rays based on the new
EAS observable - spectra of local density of muons measured at ground level in a wide
range of zenith angles - is considered. It is shown that muon density spectra are
sensitive to the primary cosmic ray spectrum and composition, and to features of the
forward kinematic region of hadronic interaction, and thus provide new information
that can be used for verification of some hypotheses about UHE cosmic ray spectra and
of EAS simulation tools. For illustration of possibilities of the new approach, the
experimental data on muon bundles at zenith angles from 30 degrees to horizon
obtained with the Russian-Italian coordinate-tracking detector DECOR are used. The
analysis based on CORSIKA simulation shows that measurements of muon density spectra
in inclined EAS give the possibility to study characteristics of primary cosmic ray
flux in a wide energy range from 10^15 to 10^19 eV by means of a single relatively
not large detector with a single experimental technique.</abstract>
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