Report on scipost_202207_00031v1

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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.authorPedro Miranda
dc.contributor.authorT. Naito
dc.contributor.authorE. Ortiz
dc.contributor.authorA. Oshima
dc.contributor.authorT. Sakai
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T21:16:54Z
dc.date.available2026-03-22T21:16:54Z
dc.date.issued2022
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/scipost.report.5530
dc.identifier.urihttps://doi.org/10.21468/scipost.report.5530
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/87006
dc.language.isoen
dc.sourceIbaraki National College of Technology
dc.subjectComputer science
dc.titleReport on scipost_202207_00031v1
dc.typepeer-review

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