dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.contributor | Universidade Estadual de Campinas (UNICAMP) | |
dc.contributor | Academy of Sciences of the URSS | |
dc.date.accessioned | 2014-05-27T11:17:25Z | |
dc.date.available | 2014-05-27T11:17:25Z | |
dc.date.created | 2014-05-27T11:17:25Z | |
dc.date.issued | 1991-03-01 | |
dc.identifier | Il Nuovo Cimento C, v. 14, n. 2, p. 145-151, 1991. | |
dc.identifier | 0390-5551 | |
dc.identifier | http://hdl.handle.net/11449/64120 | |
dc.identifier | 10.1007/BF02509394 | |
dc.identifier | 2-s2.0-51649153028 | |
dc.description.abstract | To 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.language | eng | |
dc.relation | Il Nuovo Cimento C | |
dc.rights | Acesso restrito | |
dc.source | Scopus | |
dc.subject | Other topics on the solar system | |
dc.title | Atmospheric cosmic rays in the South Atlantic anomaly region | |
dc.type | Artículos de revistas | |