4
Conferences
false
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ICN-UNAM
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3
icrc2007@icrc2007.unam.mx
30th International Cosmic Ray Conference
The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.
True
Merida, Mexico
2007-07-03T08:00:00
2007-07-11T19:00:00
2005-09-26T05:04:53
2024-04-12T17:46:55
Mexico/General
Dr.
IGeof-UNAM
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837
false
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050 (3A)
1
Poster
Lateral Distribution Functions for the Energy Estimation of UHECR Protons
Dr.
Research and Scientific Support Department of ESA ESTEC, Noordwijk
df4985b7689eff515c8c41fef4fe7d14
Prof.
Nuclear and Particle Physics Department, University of Athens
48a1771551ac274c7aaa96e4d5bdc617
Prof.
Physics Department, School of Applied Sciences, NTUA
f1ec75356a662cc803c3f575d2b9f2cd
Prof.
Physics Department, School of Applied Sciences, NTUA
ff5399857c84950d814aaaee2df8ffcc
Ms.
Physics Department, Section of Astrophysics, Astron. and Mech., Athens University
19b44a6d4904247a418215fd7695f28b
Ms.
Nuclear and Particle Physics Department, University of Athens
fd29e24fba41bb2b7381c8ba851622f5
Dr.
Research and Scientific Support Department of ESA ESTEC, Noordwijk
df4985b7689eff515c8c41fef4fe7d14
Merida, Mexico
Regency (Hyatt)
2007-07-04T14:45:00
2007-07-04T14:45:00
The energy is among the characteristics of Ultra High Energy Cosmic Rays
(E>5 x 1019 eV) which could be estimated experimentally. The following paper
attempts to estimate the energy of an UHECR proton by applying a Monte Carlo
simulation code. A number of extensive air showers, vertical and inclined,
is simulated to derive the Lateral Distribution Functions of the shower muons.
The scenario of simulations is adopted to the Cerenkov surface detector of the
P. AUGER Observatory.
Due to the fact that the Lateral Distribution Functions show minimal fluctuations
of the muon density at a distance larger than 800 m from the core of the
showers,
and due to the fact that at a distance of 900 m the distribution functions for
inclined showers coincide (which means that it does not change with the zenith
angle of the showers), we select the muon density at 900 m to derive
the energy of the primary protons.
(The project is co-funded by the European Social Fund and National
Resources (EPEAEK II) PYTHAGORAS II.)
paper
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poster
Poster
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1
More information about the venue
http://www.icrc2007.unam.mx/
link
http://www.icrc2007.unam.mx/
doc
http://indico.nucleares.unam.mx/images/word.png
word file
ppt
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pdf
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other
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link
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