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- W1993761423 abstract "Further calculations are reported on the problem of the distribution in size of cosmic-ray showers. In textsection{}2 it is shown that this distribution is completely determined when the average energy distribution of the particles in a shower is known. In textsection{}3 previous calculations of the fluctuation in size of showers have been revised and extended. The main result is that for the simplified model chosen (the so-called Furry model) the fluctuations are small and roughly equal to twice the Poisson value for all values of the thickness (see Table II; Fig. 3). In textsection{}4 another simplified model is considered for which it is possible to take the ionization exactly into account. In textsection{}5 and textsection{}6 the calculations of the fluctuation are extended to the actual cosmicray problem. For one value of the initial energy and for one depth a numerical calculation has been made (see Table III). The result for the fluctuation is again a few times the Poisson value." @default.
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- W1993761423 date "1942-12-01" @default.
- W1993761423 modified "2023-09-27" @default.
- W1993761423 title "On the Theory of Cosmic-Ray Showers II. Further Contributions to the Fluctuation Problem" @default.
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- W1993761423 doi "https://doi.org/10.1103/physrev.62.497" @default.
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