Observations of Extensive Air Showers near the Maximum of Their Longitudinal Development

dc.contributor.authorJ. Hersil
dc.contributor.authorI. Escobar
dc.contributor.authorD. Scott
dc.contributor.authorG. Clark
dc.contributor.authorS. Olbert
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T14:02:46Z
dc.date.available2026-03-22T14:02:46Z
dc.date.issued1961
dc.descriptionCitaciones: 89
dc.description.abstractExtensive air showers were studied at an altitude of 4200 m with an array of 11 scintillation detectors, and approximately 400 showers with sizes)15 x 10/sup 6/ particles were selected for detailed analysis. The function used in the analysis was the Greisen representation of the Nishimura-Kamata function. The ratios of the observed particle densities to the densities calculated from the trial function were plotted vs. distance from the core; the graphs indicate that the steepness of the lateral distribution decreases with the zenith angle. The integral intensities S of showers with sizes greater than N were then plotted vs. sec theta , and it is found that S for N near 30 x 10/sup 6/ is approximately constant for changes in sec theta near sec theta = 1, corresponding to maximum longitudinal development of showers with N approximately 30 x 10/sup 6/. A graph presenting the variation of N with x (slant thickness of atmosphere) at fixed S is also presented. (D.L.C.)
dc.identifier.doi10.1103/physrevlett.6.22
dc.identifier.urihttps://doi.org/10.1103/physrevlett.6.22
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/44221
dc.language.isoen
dc.publisherAmerican Physical Society
dc.relation.ispartofPhysical Review Letters
dc.sourceHigher University of San Andrés
dc.subjectPhysics
dc.subjectNuclear physics
dc.subjectEnvironmental science
dc.subjectAtmospheric sciences
dc.subjectMeteorology
dc.titleObservations of Extensive Air Showers near the Maximum of Their Longitudinal Development
dc.typearticle

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