“…The threshold fluence for the formation of observable damage in this study was between 5 x 10^2 and 1 X 1023 neutrons m"^ (E > 1 Me¥) for irradiation temperatures of '-eO^C (333 K). Similar damage and fluence dependence were also reported by Bryner [28] . A subsequent Investigation by Eyre and Bartlett [29] demonstrated that the "black-spot" damage consisted of point defect clusters.…”
“…The threshold fluence for the formation of observable damage in this study was between 5 x 10^2 and 1 X 1023 neutrons m"^ (E > 1 Me¥) for irradiation temperatures of '-eO^C (333 K). Similar damage and fluence dependence were also reported by Bryner [28] . A subsequent Investigation by Eyre and Bartlett [29] demonstrated that the "black-spot" damage consisted of point defect clusters.…”
“…Movement of the point defects to dislocations or their aggregation into small dislocation loops would result in annealing of the induced anisotropy and a return of magnetic properties to pre-irradiation values. A change in the distribution of point defects from uniform dispersal to aggregation into small dislocation loops would also be in agreement with electron-transmission microscopy observations of lattice damage in irradiated metals by DowNEY andEYRE (1965) andBRYNER (1966).…”
The effects of neutron irradiation on remanent magnetization in multidomain iron and kamacite (3 wt% Ni) samples of varying initial coercivities were investigated in order to determine whether cosmic ray exposure significantly affects the natural remanent magnetization (NMR) of lunar samples and chondritic meteorites. Irradiation to 1017 fast neutrons/cm2 increased bulk coercive force (He) by an average of 150. Annealing for 1 hour at 200-300C returned Hc to its pre-irradiation value. The dominant effect of irradiation on remanent magnetization was to decrease the total intensity by 5-45%. AF demagnetization spectra of both isothermal and thermal remanence before and after irradiation indicate that neutron bombardment slightly increases the resistance to AF demagnetization. No similar increase in resistance to thermal demagnetization was indicated. The changes in Hc and AF demagnetization spectra are attributed to radiation induced point defects rather than to pinning of domain walls by vacancy clusters and dislocations. The NRM in chondritic meteorites and most lunar samples is too stable to be accounted for by exposure of isothermal remanence to cosmic rays. Thus the NRM must be some form of thermal or thermochemical remanence.
“…These small clusters have been detected by other techniques of atom probe microscopy, small angle neutron scattering, and positron annihilation. Also, coarsened clusters can be seen in TEM if the material is post-irradiation annealed to a temperature of 300-400 o C [34][35][36] or if the material is irradiated at 290 o C [37,38]. At such higher temperatures thermal diffusion processes are enhanced and are sufficient to enable the clusters to grow to visible sizes.…”
Section: Discussion Of Phase 1 and 2 Findingsmentioning
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