Galactic Magnetic Field Structure and Ultra High Energy Cosmic Ray Propagation

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dc.creatorO'Neill, Sean
dc.creatorOlinto, Angela V.
dc.creatorBlasi, Pasquale
dc.date2001-08-24
dc.date.accessioned2026-07-07T01:59:45Z
dc.date.available2026-07-07T01:59:45Z
dc.descriptionWe consider the effects of the Galactic magnetic field on the propagation of ultra high energy cosmic rays (UHECRs). By employing two methods of trajectory simulation, we investigate the possibility that UHECRs are produced within the Galaxy with paths strongly influenced by the Galactic magnetic field. Such trajectories have the potential to reconcile the existing conflict between proposed local sources and isotropic UHECR arrival directions.
dc.description4 Pages, 6 Figures, Proceedings of the 27th ICRC
dc.identifierhttps://arxiv.org/abs/astro-ph/0108401
dc.identifierhttp://arxiv.org/abs/astro-ph/0108401
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3239
dc.subjectAstrophysics
dc.titleGalactic Magnetic Field Structure and Ultra High Energy Cosmic Ray Propagation
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