Atmospheric Eletric Field on Cosmic Rays Rate

dc.contributor.authorRonald Winkelmann
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T17:49:53Z
dc.date.available2026-03-22T17:49:53Z
dc.date.issued2011
dc.description.abstractFrom the moment of their formation all particles produced by a primary cosmic ray are influenced by atmospheric conditions, such as pressure, temperature, air density, and others. Atmospheric Electric Field (AEF) is one of these factors. There is evidence of a considerable increase of the counting rate of particles during electrical storms. In the present work at the Chacaltaya Cosmic Rays Physics Laboratory (5220 m a.s.l.), the existent relation between AEF and secondary particles produced by primary cosmic rays under two different weather conditions is searched, during fair weather days and disturbed weather days.
dc.identifier.doi10.22323/1.118.0053
dc.identifier.urihttps://doi.org/10.22323/1.118.0053
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/66505
dc.language.isoen
dc.sourceHigher University of San Andrés
dc.subjectCosmic ray
dc.subjectPhysics
dc.subjectCOSMIC cancer database
dc.subjectAtmospheric pressure
dc.subjectAtmospheric sciences
dc.subjectElectric field
dc.subjectAstrophysics
dc.subjectEnvironmental science
dc.subjectAstronomy
dc.titleAtmospheric Eletric Field on Cosmic Rays Rate
dc.typearticle

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