16 research outputs found
Identification, isolation, and characterization of a novel type of Fukushima-derived microparticle
In the course of the Fukushima nuclear accident, radionuclides were released in various forms, including so-called radiocesium-bearing microparticles (CsMP). So far, four types of CsMP were described: Type A is smaller in size ( 100 μm). In this work, we present a novel type of CsMP (proclaimed Type E). Three particles of Type E were extracted from a contaminated blade of grass that was sampled 1.5 km from the Fukushima Daiichi nuclear power plant in late 2011. They were located using autoradiography, isolated using an optical microscope and micromanipulator, and characterized using scanning electron microscopy, energy dispersive x-ray spectroscopy, and low-level gamma-ray spectrometry. Type E CsMPs are 10–20 μm in size and exhibit an unusually low and barely detectable 137Cs activity of only ≤ 10 mBq per particle. Their brittle and fragile character may indicate a high surface tension
Extended chondrule formation intervals in distinct physicochemical environments: Evidence from Al-Mg isotope systematics of CR chondrite chondrules with unaltered plagioclase
A temporal shift of chondrule generation from the inner to outer Solar System inferred from oxygen isotopes and Al-Mg chronology of chondrules from primitive CM and CO chondrites
Practical Utilization of Uranium-Containing Particulate Test Samples for SEM/EDS and SIMS Automated Particle Analysis Method Validation
Towards the Synthesis of Mixed Actinide Particulate Reference Materials: Microscopy and Spectroscopic Characterization of U/Ce-containing Specimens
Corrigendum to “A link between oxygen, calcium and titanium isotopes in 26Al-poor hibonite-rich CAIs from Murchison and implications for the heterogeneity of dust reservoirs in the solar nebula” [Geochim. Cosmochim. Acta 189 (2016) 70–95]
Fall, classification, and exposure history of the Mifflin L5 chondrite
The Mifflin meteorite fell on the night of April 14, 2010, in southwestern Wisconsin. A bright fireball was observed throughout a wide area of the midwestern United States. The petrography, mineral compositions, and oxygen isotope ratios indicate that the meteorite is a L5 chondrite fragmental breccia with light/dark structure. The meteorite shows a low shock stage of S2, although some shock-melted veins are present. The U,Th-He age is 0.7Ga, and the K-Ar age is 1.8Ga, indicating that Mifflin might have been heated at the time of the 470Ma L-chondrite parent body breakup and that U, Th-He, and K-Ar ages were partially reset. The cosmogenic radionuclide data indicate that Mifflin was exposed to cosmic rays while its radius was 3065cm. Assuming this exposure geometry, a cosmic-ray exposure age of 25 +/- 3Ma is calculated from cosmogenic noble gas concentrations. The low 22Ne/21Ne ratio may, however, indicate a two-stage exposure with a longer first-stage exposure at high shielding. Mifflin is unusual in having a low radiogenic gas content combined with a low shock stage and no evidence of late stage annealing; this inconsistency remains unexplained
Oxygen Isotope and Fluorine Impurity Signatures during the Conversion of Uranium Ore Concentrates to Nuclear Fuel
Within the front end of the nuclear fuel cycle, many
processes
impart forensic signatures. Oxygen-stable isotopes (δ18O values) of uranium-bearing materials have been theorized to provide
the processing and geolocational signatures of interdicted materials.
However, this signature has been minimally utilized due to a limited
understanding of how oxygen isotopes are influenced during uranium
processing. This study explores oxygen isotope exchange and fractionation
between magnesium diuranate (MDU), ammonium diuranate (ADU), and uranyl
fluoride (UO2F2) with steam (water vapor) during
their reduction to UOx. The MDU was precipitated
from two water sources, one enriched and one depleted in 18O. The UO2F2 was precipitated from a single
water source and either directly reduced or converted to ADU prior
to reduction. All MDU, ADU, and UO2F2 were reduced
to UOx in a 10% hydrogen/90% nitrogen
atmosphere that was dry or included steam. Powder X-ray diffraction
(p-XRD) was used to verify the composition of materials after reduction
as mixtures of primarily U3O8, U4O9, and UO2 with trace magnesium and fluorine
phases in UOx from MDU and UO2F2, respectively. The bulk oxygen isotope composition
of UOx from MDU was analyzed using fluorination
to remove the lattice-bound oxygen, and then O2 was subsequently
analyzed with isotope ratio mass spectrometry (IRMS). The oxygen isotope
compositions of the ADU, UO2F2, and the resulting
UOx were analyzed by large geometry secondary
ion mass spectrometry (LG-SIMS). When reduced with steam, the MDU,
ADU, and UO2F2 experienced significant oxygen
isotope exchange, and the resulting δ18O values of
UOx approached the values of the steam.
When reduced without steam, the δ18O values of converted
ADU, U3O8, and UOx products remained similar to those of the UO2F2 starting material. LG-SIMS isotope mapping of F impurity abundances
and distributions showed that direct steam-assisted reduction from
UO2F2 significantly removed F impurities while
dry reduction from UO2F2 led to the formation
of UOx that was enhanced in F impurities.
In addition, when UO2F2 was processed via precipitation
to ADU and calcination to U3O8, F impurities
were largely removed, and reductions to UOx with and without steam each had low F impurities. Overall, these
findings show promise for combining multiple signatures to predict
the process history during the conversion of uranium ore concentrates
to nuclear fuel