3-11 July 2007
Merida, Mexico
Mexico/General timezone
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Contribution Poster (WITHDRAWN)

About gamma-families fraction produced by primary protons.

Speakers

  • Prof. Toymas YULDASHBAEV

Primary authors

Co-authors

Abstract content

Primary Cosmic Ray (PCR) Mass Composition analysis performed on the basis of Pamir Collaboration X-Ray Emulsion Chambers (XREC) data. A number of selection criteria of gamma - families initiated by primary protons are considered by Tashkent group. It is shown that the fraction of registered gamma-families, originating from primary PA-interaction, consist of ~ 70-80 % at the energies Eest ~ 10 PeV and essentially decrease up to value 30-40 % above ~ 70 PeV.