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Evaluation of the flux of CR nuclei inside the magnetosphere

Authors :
Boella, G
Boschini, M
Gervasi, M
Grandi, D
Pensotti, S
Rancoita, P
Bobik, P
Kudela, K
BOELLA, GIULIANO FILIPPO
GERVASI, MASSIMO
PENSOTTI, SIMONETTA
Rancoita, PG
Kudela, K.
Boella, G
Boschini, M
Gervasi, M
Grandi, D
Pensotti, S
Rancoita, P
Bobik, P
Kudela, K
BOELLA, GIULIANO FILIPPO
GERVASI, MASSIMO
PENSOTTI, SIMONETTA
Rancoita, PG
Kudela, K.
Publication Year :
2008

Abstract

We have evaluated Cosmic Ray trajectories inside the magnetosphere and defined a Transmission Function (TF) for the CR penetration. We have then computed the TF for Helium, Carbon and Iron nuclei. Finally the flux of primary CR Helium, Carbon and Iron has been evaluated inside the magnetosphere. The results have then been compared with calculations for protons and also with experimental data collected by AMS-01 and HEAO-3

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1311385603
Document Type :
Electronic Resource