Proton Dominance of Sub-LET Threshold GCR SEE Rate
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...
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| Veröffentlicht in: | IEEE transactions on nuclear science 2017-01, Vol.64 (1), p.388-397 |
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| creator | Alia, Ruben Garcia Brugger, Markus Ferlet-Cavrois, Veronique Brandenburg, Sytze Calcutt, Jordan Cerutti, Francesco Daly, Eamonn Ferrari, Alfredo Muschitiello, Michele Santin, Giovanni Uznanski, Slawosz Van Goethem, Marc-Jan Zadeh, Ali |
| description | 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. |
| doi_str_mv | 10.1109/TNS.2016.2628363 |
| format | Article |
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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.</description><identifier>ISSN: 0018-9499</identifier><identifier>EISSN: 1558-1578</identifier><identifier>DOI: 10.1109/TNS.2016.2628363</identifier><identifier>CODEN: IETNAE</identifier><language>eng</language><publisher>New York: IEEE</publisher><subject>Abundance ; Cosmic rays ; Energy ; FLUKA ; Galactic cosmic rays ; Heavy ions ; indirect ionization ; Ionization ; Monte Carlo methods ; MOSFET ; nuclear reactions ; Protons ; radiation hardness assurance ; Random access memory ; Reaction products ; Single Event Effects ; single-event burnout (SEB) ; single-event latchup (SEL) ; single-event upset (SEU)</subject><ispartof>IEEE transactions on nuclear science, 2017-01, Vol.64 (1), p.388-397</ispartof><rights>Copyright The Institute of Electrical and Electronics Engineers, Inc. (IEEE) 2017</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c372t-29583f89c9b12684544f21189dce3480e9699a2c53d17019b019175c31ab363a3</citedby><cites>FETCH-LOGICAL-c372t-29583f89c9b12684544f21189dce3480e9699a2c53d17019b019175c31ab363a3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/7742933$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>314,780,784,796,27924,27925,54758</link.rule.ids><linktorsrc>$$Uhttps://ieeexplore.ieee.org/document/7742933$$EView_record_in_IEEE$$FView_record_in_$$GIEEE</linktorsrc></links><search><creatorcontrib>Alia, Ruben Garcia</creatorcontrib><creatorcontrib>Brugger, Markus</creatorcontrib><creatorcontrib>Ferlet-Cavrois, Veronique</creatorcontrib><creatorcontrib>Brandenburg, Sytze</creatorcontrib><creatorcontrib>Calcutt, Jordan</creatorcontrib><creatorcontrib>Cerutti, Francesco</creatorcontrib><creatorcontrib>Daly, Eamonn</creatorcontrib><creatorcontrib>Ferrari, Alfredo</creatorcontrib><creatorcontrib>Muschitiello, Michele</creatorcontrib><creatorcontrib>Santin, Giovanni</creatorcontrib><creatorcontrib>Uznanski, Slawosz</creatorcontrib><creatorcontrib>Van Goethem, Marc-Jan</creatorcontrib><creatorcontrib>Zadeh, Ali</creatorcontrib><title>Proton Dominance of Sub-LET Threshold GCR SEE Rate</title><title>IEEE transactions on nuclear science</title><addtitle>TNS</addtitle><description>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. 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| subjects | Abundance Cosmic rays Energy FLUKA Galactic cosmic rays Heavy ions indirect ionization Ionization Monte Carlo methods MOSFET nuclear reactions Protons radiation hardness assurance Random access memory Reaction products Single Event Effects single-event burnout (SEB) single-event latchup (SEL) single-event upset (SEU) |
| title | Proton Dominance of Sub-LET Threshold GCR SEE Rate |
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