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• W4311399839 endingPage "8235" @default.
• W4311399839 startingPage "8205" @default.
• W4311399839 abstract "The age of exascale computing has arrived and the risks associated with neutron and other atmospheric radiation are becoming more critical as the computing power increases, hence, the expected Mean Time Between Failures will be reduced because of this radiation. In this work, a new and detailed calculation of the neutron flux for energies above 50 MeV is presented. This has been done by using state-of-the-art Monte Carlo astroparticle techniques and including real atmospheric profiles at each one of the next 23 exascale supercomputing facilities. Atmospheric impact in the flux and seasonal variations were observed and characterised, and the barometric coefficient for high-energy neutrons at each site was obtained. With these coefficients, potential risks of errors associated with the increase in the flux of energetic neutrons, such as the occurrence of single event upsets or transients, and the corresponding failure-in-time rates, can be anticipated just by using the atmospheric pressure before the assignation of resources to critical tasks at each exascale facility. For more clarity, examples about how the rate of failures is affected by the cosmic rays are included, so administrators will better anticipate which more or less restrictive actions could take for overcoming errors." @default.
• W4311399839 created "2022-12-26" @default.
• W4311399839 creator A5051116278 @default.
• W4311399839 creator A5061081759 @default.
• W4311399839 date "2022-12-14" @default.
• W4311399839 modified "2023-09-29" @default.
• W4311399839 title "Calculation of the high-energy neutron flux for anticipating errors and recovery techniques in exascale supercomputer centres" @default.
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