4
Conferences
false
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ICN-UNAM
1482bc95ee34f0461176da21871284c8
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
40af9343b8bb9d18708b4f0252d5f53c
888
false
[["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]]
052 (3A)
1
Poster
Nuclear Cosmic Ray Propagation in the Atmosphere between 10GeV and 10TeV per nucleon
Dr.
LPSC/IN2P3/CNRS
5e7909e96ba4af50b6f8f7be99d09b75
Dr.
LPSC/IN2P3/CNRS
5e7909e96ba4af50b6f8f7be99d09b75
Ms.
LPSC/IN2P3/CNRS
de2d457f4c842e24e3ca80c47358a64c
Dr.
LPNHE/IN2P3/CNRS
b42a3b55979c6cecf073ab5e242a1eab
Dr.
LPSC/IN2P3/CNRS
6dafde39119745f684eb6c0cf2372883
Merida, Mexico
Regency (Hyatt)
2007-07-06T14:45:00
2007-07-06T14:45:00
The future high energy nuclear cosmic ray flux measurements in the upper atmosphere
will require large, and thus accurate, corrections for reliable Top of Atmosphere
(galactic) fluxes to be derived. In this perspective, the atmospheric corrections are
evaluated from the transport calculations of the flux in the atmosphere. The
contributions of these corrections to the accuracy of the experimental results are
discussed for the B/C and subFe/Fe elements ratios, over the kinetic energy range 10
- 10**4 GeV/n. These contributions become largely dominant at the highest energies
investigated. The results and the prospects for the galactic flux measurements will
be discussed in the presentation.
paper
doc
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word file
ppt
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powerpoint file
pdf
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pdf file
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presentation file
ods
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link
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link
1
More information about the venue
http://www.icrc2007.unam.mx/
link
http://www.icrc2007.unam.mx/
doc
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word file
ppt
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pdf
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pdf file
odt
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presentation file
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spreadsheet file
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link
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link