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For the majority of the samples the Ne Ne and

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For the majority of the samples, the 20Ne/22Ne and 36Ar/40Ar ratios agree or GS7340 very close to the ASW values. As diffusion-controlled Ne and Ar isotope fractionation in not evident, the observed noble-gas depletion can conceptually be understood in terms of loss of a gas phase being equilibrated with the surrounding pore water phase.
Such gas loss can be corrected as described for the case of organic-rich lacustrine sediments in Soppensee using a 1-step-degassing model (Brennwald et al., 2005). The 1-step-degassing model calculates the noble-gas concentration in the pore water after equilibration with a gas phase as Ci = Ci∗/(1 + B·Hi/P0) using the expected atmospheric equilibrium concentration Ci∗ (with i = Ne, Ar, Kr, Xe), the STP bubble volume per unit mass of pore water B, the Henry coefficient Hi for noble gas i (corrected for the specific hydrochemistry of Lake Van, see Section 3.2), and the STP dry-gas pressure P0.
We based our degassing correction on Ne, Ar, Kr, and Xe. We estimated B (i.e., the variable parameterising gas loss) for each sample by least-square fitting of the concentrations predicted by the degassing model to the measured noble gas concentrations (Fig. 3; for further details see Brennwald et al., 2005). The error for B is mass extinction calculated from the deviations of the modelled concentrations with respect to the measured concentrations. The estimation of B is used to calculate the original He concentration in the pore water (i.e., prior to equilibration with the gas phase).

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