High-Energy Electron-Induced SEUs and Jovian Environment Impact
We present experimental evidence of electron-induced upsets in a reference European Space Agency (ESA) single event upset (SEU) monitor, induced by a 200-MeV electron beam at the Very energetic Electronic facility for Space Planetary Exploration in harsh Radiation environments facility at CERN. Comp...
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| Veröffentlicht in: | IEEE transactions on nuclear science 2017-08, Vol.64 (8), p.2016-2022 |
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| container_end_page | 2022 |
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| container_issue | 8 |
| container_start_page | 2016 |
| container_title | IEEE transactions on nuclear science |
| container_volume | 64 |
| creator | Tali, Maris Alia, Ruben Garcia Brugger, Markus Ferlet-Cavrois, Veronique Corsini, Roberto Farabolini, Wilfrid Mohammadzadeh, Ali Santin, Giovanni Virtanen, Ari |
| description | We present experimental evidence of electron-induced upsets in a reference European Space Agency (ESA) single event upset (SEU) monitor, induced by a 200-MeV electron beam at the Very energetic Electronic facility for Space Planetary Exploration in harsh Radiation environments facility at CERN. Comparison of experimental cross sections and simulated cross sections is shown and the differences are analyzed. Possible secondary contributions to the upset rate by neutrons, flash effects, and cumulative dose effects are discussed, showing that electronuclear reactions are the expected SEU mechanism. The ESA Jupiter Icy Moons Explorer mission, to be launched in 2022, presents a challenging radiation environment due to the intense high-energy electron flux in the trapped radiation belts. Insight is given to the possible contribution of electrons to the overall upset rates in the Jovian radiation environment. Relative contributions of both typical electron and proton spectra created when the environmental spectra are transported through a typical spacecraft shielding are shown and the different mission phases are discussed. |
| doi_str_mv | 10.1109/TNS.2017.2713445 |
| format | Article |
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Comparison of experimental cross sections and simulated cross sections is shown and the differences are analyzed. Possible secondary contributions to the upset rate by neutrons, flash effects, and cumulative dose effects are discussed, showing that electronuclear reactions are the expected SEU mechanism. The ESA Jupiter Icy Moons Explorer mission, to be launched in 2022, presents a challenging radiation environment due to the intense high-energy electron flux in the trapped radiation belts. Insight is given to the possible contribution of electrons to the overall upset rates in the Jovian radiation environment. 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Comparison of experimental cross sections and simulated cross sections is shown and the differences are analyzed. Possible secondary contributions to the upset rate by neutrons, flash effects, and cumulative dose effects are discussed, showing that electronuclear reactions are the expected SEU mechanism. The ESA Jupiter Icy Moons Explorer mission, to be launched in 2022, presents a challenging radiation environment due to the intense high-energy electron flux in the trapped radiation belts. Insight is given to the possible contribution of electrons to the overall upset rates in the Jovian radiation environment. 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| subjects | Cross-sections Dosage Electron beams Electron density Electrons Energy Environmental impact Icy satellites Jupiter Jupiter satellites Laser beams Measurement by laser beam Monitoring Monte Carlo methods Neutron flux Neutrons Photonics Protons Radiation Radiation belts radiation effects Radiation shielding Single event upsets Space exploration Spacecraft Spacecraft shielding |
| title | High-Energy Electron-Induced SEUs and Jovian Environment Impact |
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