Proton-air inelastic cross section at S(1/2) = 30 TeV

Details Proton-air inelastic cross section at S(1/2) = 30 TeV Proton-air inelastic cross section at S(1/2) = 30 TeV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6....5b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 5-8 (SEE N85-35848 24-93)

Physics

1

Air, Cosmic Ray Showers, Energy Spectra, Inelastic Scattering, Protons, Scattering Cross Sections, Center Of Mass, Cerenkov Radiation, Fluorescence, Flux Density, Normal Density Functions, Photomultiplier Tubes, Radiation Detectors, Radiation Distribution

Scientific paper

The authors have measured the distribution of the maxima of high energy
cosmic ray induced extensive air showers in the atmosphere as a function
of atmospheric depth. From the exponential tail of this distribution,
they determined the p-air inelastic cross section at 30 TeV
center-of-mass energy to be 540±40 mb.

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