Status of the world-wide network of solar neutron telescopes in solar cycle 24

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dc.contributor.authorY. Matsubara
dc.contributor.authorY. Muraki
dc.contributor.authorT. Sako
dc.contributor.authorY. Itow
dc.contributor.authorT. Sakai
dc.contributor.authorS. Shibata
dc.contributor.authorT. Yuda
dc.contributor.authorM. Ohnishi
dc.contributor.authorH. Tsuchiya
dc.contributor.authorY. Katayose
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T16:45:17Z
dc.date.available2026-03-22T16:45:17Z
dc.date.issued2009
dc.descriptionCitaciones: 1
dc.description.abstractA network of solar neutron telescopes has been developed since the middle of solar cycle 22. We have detected several important solar neutron events until the end of solar cycle 23 using solar neutron telescopes, but the accumulation of more solar neutron events is indispensable to eclucidate the acceleration mechanism of high energy particles. The data of the solar magnetic field with a space resolution of 0.3 arcsec obtained by Hinode satellite will be useful to understand solar neutron events more efficiently than during the previous solar cycles. In this paper we discuss the expected scientific results obtained by the world-wide network of solar neutron telescopes during solar cycle 24.
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/60109
dc.language.isoen
dc.sourceNagoya University
dc.subjectSolar cycle
dc.subjectPhysics
dc.subjectNeutron
dc.subjectSolar minimum
dc.subjectCoronal mass ejection
dc.subjectSolar energy
dc.subjectAstronomy
dc.titleStatus of the world-wide network of solar neutron telescopes in solar cycle 24
dc.typearticle

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