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Search for solar neutrons using NM-64 equipmentTwo 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.
Document ID
19850026452
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Martinic, N. J.
(San Andres Univ. La Paz, Bolivia)
Reguerin, A.
(San Andres Univ. La Paz, Bolivia)
Palenque, E.
(San Andres Univ. La Paz, Bolivia)
Taquichiri, M. A.
(San Andres Univ. La Paz, Bolivia)
Wada, M.
(Inst. of Physical and Chemical Research Tokyo, United States)
Inoue, A.
(Inst. of Physical and Chemical Research Tokyo, United States)
Takahashi, K.
(Inst. of Physical and Chemical Research Tokyo, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 4
Subject Category
Solar Physics
Report/Patent Number
SH-1.4-5
Report Number: SH-1.4-5
Accession Number
85N34765
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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