Proton Dominance of Sub-LET Threshold GCR SEE RateAlia, R. G., Brugger, M., Ferlet-Cavrois, V., Brandenburg, S., Calcutt, J., Cerutti, F., Daly, E., Ferrari, A., Muschitiello, M., Santin, G., Uznanski, S., Van Goethem, M-J. & Zadeh, A., Jan-2017, In : IEEE Transactions on Nuclear Science. 64, 1, p. 388-397 10 p.
Research output: Contribution to journal › Article › Academic › peer-review
We apply a Monte Carlo based integral rectangular parallel-piped (IRRP) approach to evaluate the impact of heavy ion reaction products on the Galactic Cosmic Ray (GCR) Single Event Effect (SEE) rate, concluding that owing to their similar high-energy (> 100 MeV/n) SEE cross section and much larger abundance, protons are expected to be the dominating contributor. In addition, a broad set of components, ions and energies is used to explore the sub-LET threshold experimental region for standard ground-level heavy ion test energies, identifying an overall decreasing trend in the 10-80 MeV/n range due to the decreased contribution of complete and break-up fusion, and pointing out the limitations associated to the application of Monte Carlo SEE models in this energy interval.
|Number of pages||10|
|Journal||IEEE Transactions on Nuclear Science|
|Publication status||Published - Jan-2017|
- FLUKA, indirect ionization, Monte Carlo methods, nuclear reactions, radiation hardness assurance, single-event burnout (SEB), single-event latchup (SEL), single-event upset (SEU), CROSS-SECTION, HIGH-ENERGY, FLUKA CODE, RATE PREDICTION, PROBA-II, TECHNOLOGY, CHALLENGES, DEPENDENCE, LATCHUP, IMPACT