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<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>
 <address></address>
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<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
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<modificationDate>2024-04-12T17:46:55</modificationDate>
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 <title>Lateral distribution of charged particles measured in air showers by the ARGO-YBJ experiment.</title>
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   <name first="Min" middle="" last="Zha"></name>
   <organization>IHEP, Beijing, China</organization>
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   <title>Dr.</title>
   <name first="Giuseppe" middle="" last="Di Sciascio"></name>
   <organization>INFN, Sez. Napoli, Italy</organization>
   <emailHash>f4f5c30a5f4a90bfefeb8c3efca97352</emailHash>
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  <user>
   <title>Dr.</title>
   <name first="Min" middle="" last="Zha"></name>
   <organization>IHEP, Beijing, China</organization>
   <emailHash>ad831b3f298c39c114b06a2b4ac01be6</emailHash>
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   <title>Dr.</title>
   <name first="Xiangdong" middle="" last="Sheng"></name>
   <organization>IHEP, Beijing, China</organization>
   <emailHash>e871a60326ff86363c3ec816ae064f77</emailHash>
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   <name first="Carlo" middle="" last="Vigorito"></name>
   <organization>INFN, Sez. Torino, Italy</organization>
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 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
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 <abstract>The ARGO-YBJ experiment, installed at the YangBaJing Cosmic Ray
Laboratory (4300 m a.s.l., Tibet, P.R. China), is an air shower
array exploiting the full coverage approach at very high altitude.
Signals from each RPC are picked-up by strips 6 cm wide and 62 cm
long, thus allowing to sample the Extensive Air Showers (EAS) with
an unprecedented granularity. In order to extend the dynamic range
up to PeV energies, a charge read-out has been implemented by
instrumenting every RPC also with two large size pads of dimension
140$\times$125 cm$^2$ each. As a consequence, for the first time
the topological characteristics of EAS and the geometric structure
of shower cores can be investigated with a great detail over more
than two energy decades, up to the knee region.

In this work we report a measurement of the lateral distribution
of charged particles in EAS performed by the ARGO-YBJ carpet. The
sensitivity to the primary mass at energies higher than 10$^{14}$
eV will be discussed. A procedure to select events characterized
by unusual distributions of charged particles (multicore events,
aligned structures, "halo" events, etc.) will be also presented.</abstract>
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