In the space environment, instruments onboard of spacecrafts can be affected by displacement damage due to radiation. The differential scattering cross section for screened nucleus–nucleus interactions - i.e., including the effects due to screened Coulomb nuclear fields -, nuclear stopping powers and non-ionization energy losses are treated from about 50 keV/nucleon up to relativistic energies.

Boschini, M., Consolandi, C., Gervasi, M., Giani, S., Grandi, D., Ivantchenko, V., et al. (2011). Nuclear and non-ionizing energy-loss for Coulomb scattered particles from low energy up to relativistic regime in space radiation environment. In ICATPP Conference on Cosmic Rays for Particle and Astroparticle Physics (pp.9-23). World Scientific [10.1142/9789814329033_0002].

Nuclear and non-ionizing energy-loss for Coulomb scattered particles from low energy up to relativistic regime in space radiation environment

CONSOLANDI, CRISTINA;GERVASI, MASSIMO;Grandi, D;PENSOTTI, SIMONETTA;TACCONI, MAURO
2011

Abstract

In the space environment, instruments onboard of spacecrafts can be affected by displacement damage due to radiation. The differential scattering cross section for screened nucleus–nucleus interactions - i.e., including the effects due to screened Coulomb nuclear fields -, nuclear stopping powers and non-ionization energy losses are treated from about 50 keV/nucleon up to relativistic energies.
paper
Radiation damage; NIEL
English
ICATPP Conference on Cosmic Rays for Particle and Astroparticle Physics
2010
Giani, S; Leroy, C; Rancoita, PG
ICATPP Conference on Cosmic Rays for Particle and Astroparticle Physics
9814329026
2011
6
9
23
none
Boschini, M., Consolandi, C., Gervasi, M., Giani, S., Grandi, D., Ivantchenko, V., et al. (2011). Nuclear and non-ionizing energy-loss for Coulomb scattered particles from low energy up to relativistic regime in space radiation environment. In ICATPP Conference on Cosmic Rays for Particle and Astroparticle Physics (pp.9-23). World Scientific [10.1142/9789814329033_0002].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/39065
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