2015
DOI: 10.1109/tns.2015.2498103
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Terrestrial Muon Flux Measurement at Low Energies for Soft Error Studies

Abstract: A large volume scintillator detector has been used to measure the terrestrial stopping muon rate under different conditions of location, altitude, shielding and weather to determine the range of variation of the low energy muon flux. About 1 year of data has been collected under different conditions. This data can then be used to compare with cosmic ray muon simulations and to estimate the soft error rate due to direct ionization of muons.

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Cited by 9 publications
(6 citation statements)
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“…In particular, these studies have highlighted the differences between the effects of positive and negative muons on SRAM memories, also as a function of their energy. All these experimental results under beam conditions, together with other previous works [15][16][17], show or suggest that in practice only a small fraction of atmospheric muons are likely to be a potential threat to electronics-especially those with low energies, typically below a few MeV. This is because the average stopping power of atmospheric muons is significantly lower than that of protons, alpha particles, or heavy ions.…”
Section: Introductionmentioning
confidence: 54%
See 1 more Smart Citation
“…In particular, these studies have highlighted the differences between the effects of positive and negative muons on SRAM memories, also as a function of their energy. All these experimental results under beam conditions, together with other previous works [15][16][17], show or suggest that in practice only a small fraction of atmospheric muons are likely to be a potential threat to electronics-especially those with low energies, typically below a few MeV. This is because the average stopping power of atmospheric muons is significantly lower than that of protons, alpha particles, or heavy ions.…”
Section: Introductionmentioning
confidence: 54%
“…Figure 7 shows the distribution in number of all light-charged particles and fragment nuclei as a function of their atomic number. For Z = 1, the products include protons (94,235), deuterons (15,381), and tritons (3309); for Z = 2, the products include alpha particles (42,576) and 3 He nuclei (339). Beryllium (Z = 4) appears as the least-produced nucleus (764), followed by oxygen (1275), boron (1467), and fluorine (1620).…”
Section: Case Of Natural Siliconmentioning
confidence: 99%
“…Atmospheric and terrestrial neutron, proton, μ ± spectra were used. The spectra were evaluated through the FLUKA Galactic Cosmic Rays (GCR) simulations summarized in section II and benchmarked, against reference data [5] and experimental measurements [26]. Spectra were evaluated in the area of Vancouver (49 • 15' 0" N 123 • 8' 0" W) in the 1 keV-10 TeV energy range (10 −5 eV-10 TeV for neutron) at different atmospheric depths (1033 g/cm 2 , 909 g/cm 2 and 211 g/cm 2 ).…”
Section: B Source Particle Spectramentioning
confidence: 99%
“…Work in Ref. [20] uses large area plastic scintillator and gives the energy spectra of passing and stopping muons and decay electrons/positrons at ground and at depth. There are several recent works using plastic scintillators to measure muon angle distributions using plastic scintillator bars [21,22].…”
Section: Introductionmentioning
confidence: 99%