Search for solar neutrons using NM-64 equipment

dc.contributor.authorN. Martinić
dc.contributor.authorA. Reguerín
dc.contributor.authorEduardo Palenque
dc.contributor.authorM. A. Taquichiri
dc.contributor.authorM. Wada
dc.contributor.authorA. Inoue
dc.contributor.authorKazuyoshi Takahashi
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T15:52:08Z
dc.date.available2026-03-22T15:52:08Z
dc.date.issued1985
dc.descriptionCitaciones: 3
dc.description.abstractTwo years (1980 to 1982) neutron monitor data from the Chacaltaya (geographic coordinates: N16.32 deg W68. 15 deg; cutoff rigidity: 13.1 GV; altitude: 5,300 m a.s.l.) station has been scanned; the sampling time of the 12NM-64 neutron monitor is 5 min. The nucleonic component increases have been correlated with 66 hard X-, gamma rays satellite data from solar origin, as reported by several groups. Typical neutron monitor time profiles of the events are presented. Chree-analysis was performed discriminating the events according to its solar coordinates. Ground data from solar limb locii are more enhanced at the time of the onset than other geometrically visible flares. Chree histograms of neutron monitor output profiles are also presented from geometrically invisible events from the Chacaltaya station.
dc.identifier.urihttps://ntrs.nasa.gov/api/citations/19850026452/downloads/19850026452.pdf
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/54886
dc.language.isoen
dc.publisherNASA Headquarters
dc.relation.ispartofNASA Technical Reports Server (NASA)
dc.sourceHigher University of San Andrés
dc.subjectNeutron monitor
dc.subjectNeutron
dc.subjectPhysics
dc.subjectRemote sensing
dc.subjectSatellite
dc.subjectAltitude (triangle)
dc.subjectOptics
dc.titleSearch for solar neutrons using NM-64 equipment
dc.typearticle

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