The Multiply Scattering Effect on the Energy Measurement of UHE Cosmic Rays using Atmospheric Fluorescence Technique

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dc.creatorZhang, Xingzhi
dc.date2000-04-12
dc.date.accessioned2026-07-07T01:53:07Z
dc.date.available2026-07-07T01:53:07Z
dc.descriptionPoint sources in the atmosphere are surrounded by aureole because of atmospheric scattering. The properties of the time-dependent aureole radiance are calculated by use of a Monte Carlo approach and an iterative method. Since the aureole is particularly important in the ultraviolet, which is the region the Ultra-High-Energy (UHE) cosmic ray experiment using the air fluorescence technique like Fly's Eye or High-Resolution-Fly's-Eye(HiRes) are set in. The effect of the multiply scatteing on the energy measurement is studied.
dc.description17 pages, 17 figures, submitted t astr. part. phys
dc.identifierhttps://arxiv.org/abs/astro-ph/0004173
dc.identifierhttp://arxiv.org/abs/astro-ph/0004173
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/854
dc.subjectAstrophysics
dc.titleThe Multiply Scattering Effect on the Energy Measurement of UHE Cosmic Rays using Atmospheric Fluorescence Technique
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