Proton penetration efficiency over a high altitude observatory in Mexico

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dc.contributor.authorShoko Miyake
dc.contributor.authorT. Koi
dc.contributor.authorY. Muraki
dc.contributor.authorY. Matsubara
dc.contributor.authorS. Masuda
dc.contributor.authorP. Miranda
dc.contributor.authorT. Naito
dc.contributor.authorE. Ortiz
dc.contributor.authorA. Oshima
dc.contributor.authorT. Sakai
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T15:21:39Z
dc.date.available2026-03-22T15:21:39Z
dc.date.issued2023
dc.descriptionCitaciones: 2
dc.description.abstractIn association with a large solar flare on November 7, 2004, the solar neutron detectors located at Mt. Chacaltaya (5,250 m) in Bolivia and Mt. Sierra Negra (4,600 m) in Mexico recorded very interesting events. In order to explain these events, we have performed a calculation solving the equation of motion of anti-protons inside the magnetosphere. Based on these results, the Mt. Chacaltaya event may be explained by the detection of solar neutrons, while the Mt. Sierra Negra event may be explained by the first detection of very high energy solar neutron decay protons (SNDPs) around 6 GeV.
dc.identifier.doi10.21468/scipostphysproc.13.001
dc.identifier.urihttps://doi.org/10.21468/scipostphysproc.13.001
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/51915
dc.language.isoen
dc.publisherSciPost.org
dc.relation.ispartofSciPost Physics Proceedings
dc.sourceNational Institute of Technology, Kagoshima College
dc.subjectPhysics
dc.subjectObservatory
dc.subjectNeutron
dc.subjectSolar flare
dc.subjectNuclear physics
dc.subjectProton
dc.subjectMagnetosphere
dc.subjectEffects of high altitude on humans
dc.subjectEvent (particle physics)
dc.subjectFlare
dc.titleProton penetration efficiency over a high altitude observatory in Mexico
dc.typearticle

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