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- W1999672008 abstract "The natural rates of occurrence, in the gases He, N, Ne, and A, of nuclear interactions of the cosmic ray $N$ component in which more than 8 Mev are given to charged secondary particles, have been measured. The rates per gram atom of the four gases are in about the same ratio as their geometric nuclear cross sections. An integrated flux of $N$ rays of 6.0ifmmodetimeselsetexttimesfi{}${10}^{ensuremath{-}3}$ ${mathrm{cm}}^{ensuremath{-}2}$ ${mathrm{sec}}^{ensuremath{-}1}$ would produce the observed rates of occurrence of nuclear interactions if the cross section were geometric. The rates in argon, measured at sea level and 10 600-ft elevation, correspond to an absorption mean free path in air of 132ifmmodepmelsetextpmfi{}4 g ${mathrm{cm}}^{ensuremath{-}2}$ for the total flux of $N$ rays. The interactions, 2783 in total, were observed in the gas of a cloud chamber filled to 5 atmos pressure. Inside the cloud chamber was placed a system of wires forming an ionization chamber. An expansion was initiated whenever a pulse from the ionization chamber corresponding to an energy release of more than 8 Mev (1.5 Po alpha) occurred. Fast reduction of the high voltage after electron collection was over permitted track formation on the positive ions. Of the nuclear interactions produced in argon about 20 percent are produced by charged particles at the higher elevation, and about 15 percent at sea level." @default.
- W1999672008 created "2016-06-24" @default.
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- W1999672008 date "1954-02-01" @default.
- W1999672008 modified "2023-09-26" @default.
- W1999672008 title "Cosmic-Ray Nuclear Interactions in Gases" @default.
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- W1999672008 doi "https://doi.org/10.1103/physrev.93.528" @default.
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