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Energy Transfer to Nucleons in Cosmic-Ray Stars at 95,000 Feet
Phys. Rev. 78, 680 – Published 15 June, 1950
DOI: https://doi.org/10.1103/PhysRev.78.680
Abstract
The size-frequency distribution of cosmic-ray stars produced in photographic emulsions exposed at 95,000-feet altitude and the energies associated with the non-relativistic prongs of these stars have been determined. A distribution function for the excitation energy of stars with more than 8 prongs is derived.
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