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

Boella, G., Boschini, M., Gervasi, M., Grandi, D., Pensotti, S., Rancoita, P., et al. (2008). Evaluation of the flux of CR nuclei inside the magnetosphere. In ASTROPARTICLE, PARTICLE AND SPACE PHYSICS, DETECTORS AND MEDICAL PHYSICS APPLICATIONS (pp.875-880) [10.1142/9789812819093_0146].

Evaluation of the flux of CR nuclei inside the magnetosphere

BOELLA, GIULIANO FILIPPO;GERVASI, MASSIMO;Grandi, D;PENSOTTI, SIMONETTA;
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
paper
Galactic Cosmic Rays, Magnetosphere
English
International Conference on Advanced Technology and Particle Physics October 8-12
2007
ASTROPARTICLE, PARTICLE AND SPACE PHYSICS, DETECTORS AND MEDICAL PHYSICS APPLICATIONS
978-981-281-908-6
2008
4
875
880
none
Boella, G., Boschini, M., Gervasi, M., Grandi, D., Pensotti, S., Rancoita, P., et al. (2008). Evaluation of the flux of CR nuclei inside the magnetosphere. In ASTROPARTICLE, PARTICLE AND SPACE PHYSICS, DETECTORS AND MEDICAL PHYSICS APPLICATIONS (pp.875-880) [10.1142/9789812819093_0146].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/21804
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