dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorVan Bui, N. A.
dc.creatorMartin, I. M.
dc.creatorVieira, C. A.
dc.creatorStozhkov, Yu I.
dc.creatorFradkin, M. I.
dc.date2014-05-27T11:17:25Z
dc.date2016-10-25T18:12:43Z
dc.date2014-05-27T11:17:25Z
dc.date2016-10-25T18:12:43Z
dc.date1991-03-01
dc.date.accessioned2017-04-06T00:43:12Z
dc.date.available2017-04-06T00:43:12Z
dc.identifierIl Nuovo Cimento C, v. 14, n. 2, p. 145-151, 1991.
dc.identifier0390-5551
dc.identifierhttp://hdl.handle.net/11449/64120
dc.identifierhttp://acervodigital.unesp.br/handle/11449/64120
dc.identifier10.1007/BF02509394
dc.identifier2-s2.0-51649153028
dc.identifierhttp://dx.doi.org/10.1007/BF02509394
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/886043
dc.descriptionTo study the production and propagation of fast secondaries particles in the atmosphere, data collected during eleven quiet-time balloon flights are analysed. Comparisons of these data with those obtained in different geomagnetic rigidity regions permit to estimate the contributions of the proton and electron components in the measured intensities. Derivations of this last component in the «upward» and «downward» moving electrons fluxes indicate that in the anomaly region a fraction of these particles, produced by the primary protons, are leaving the atmosphere and will not return to the Earth. © 1991 Società Italiana di Fisica.
dc.languageeng
dc.relationIl Nuovo Cimento C
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectOther topics on the solar system
dc.titleAtmospheric cosmic rays in the South Atlantic anomaly region
dc.typeOtro


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