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- W133078531 abstract "In a study of the development of extensive air showers in the atmosphere, a hodoscope experiment was carried out at three mountain stations: Chacaltaya (5,200m), Mt. Evans (4,300m), and Echo Lake (3,260m). Six trays containing a total of 80 couaters were used to determine the size and the lateral distribution of the showers. Four other trays with 54 counters and four liquid scintillators served to measure the transition effect of the shower electrons in lead, and thus to determine the age of the showers. The events could then be grouped and analyzed according to both age and size. The lateral distribution of showers of different age (as determined from the transition effect), both near the core and at larger distances, showed very little variation with altitude and with age. Near the core it is flatter than outside, and the flattening extends at all altitudes over an equal distance. Apparently this phenomenon is due to the continuous effect of the nucleonic component. The attenuation of the shower rate, at fixed geometry, is practically constant between 5,200 and 3,260m, the attenuation mean free path between Mt. Evans and Chacaltaya for the youngest showers being (155 plus or minus 12) g/cm/sup 2/ againstmore » an averange of about 140 g/cm/sup 2/. The attenuation of the particle numbers in showers of equal frequency was over the whole range exponential with a mean free path of about 125 g/cm/sup 2/. The interaction mean free path of the shower primaries, determined from a comparison of the rates of showers of equal size and age at the three stations, was (87 plus or minus 7) g/cm/sup 2/. This suggests that the shower primaries, in the energy region concerned (about 10/sup 15/ ev), are predominantly protons. (auth)« less" @default.
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- W133078531 date "1957-07-01" @default.
- W133078531 modified "2023-09-27" @default.
- W133078531 title "AIR SHOWER OBSERVATIONS BETWEEN 5,200M AND 3,260M ALTITUDE" @default.
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