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Interactions of HighEnergy Particles with Matter
7 other sections not shown
absorption abundances acceleration altitude angular distribution approximately atmospheric depth bremsstrahlung cascade showers cloud chamber Cocconi collision component Compton effect cross section curve decay decreases density detectors Dobrotin effect electrons emitted emulsion energies greater energy dependence energy loss energy spectrum estimated experimental expressed factor Fermi fireball flux frequency Galactic Galaxy geomagnetic GeV/c Hayakawa heavy nuclei Hence high energies hydrogen incident energy increases inelasticity integral intensity intergalactic interstellar ionization isotropic kaons kinetic energy low energies magnetic field mass mean free path meson momenta multiple muons neutrino neutrons nuclear active particles nuclear interactions nuclei nucleon Nuovo Cim observed obtained pair creation Phys pions primary cosmic rays primary energy Proc produced protons radiation length ratio relativistic represented Rossi scattering sea level secondary particles shown in Fig smaller solar solar cosmic rays sources spectra theory transverse momentum velocity whereas X-ray y-rays zenith angle