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Copper abundance data

The application of seismic networks for monitoring slope conditions at open-cast mines has generated abundant data in the event of slope failure. An enormous 65 x 10 m landslide occurred at the Bingham Canyon copper mine in the USA in 2013 (Pankow et al. 2014). In this case, seismometers that detected the event were located between 6 and 400 km. The landslide, classified as a rock avalanche, was actually two closely spaced events. The seismicity was dominated by long-period events with differences between the two episodes only the first one produced a high-amplitude peak near the end of the coda and there was a large difference when the maximum amplitude occurred. [Pg.2391]

Making and Using Tables Data Table 3 shows the isotopic mass and relative abundance for the most common isotopes of copper and zinc. [Pg.199]

As some necessary meteorological data were unavailable, we employed two different techniques to estimate the element abundance in air. Reverse calculations, in the framework of the American program MEPAS, allowed us to find the concentration fields based on experimental and especially adapted meteorological data. The second technique included direct calculations in the framework of the Russian standardized program Ecologist, which took into account the actual chemical composition of copper-smelting production contaminants. Both techniques had some restrictions, mainly insufficient initial information on the sources of contaminants and limited possibilities of the analytical equipment used. [Pg.139]

Figure 3. An example of correlation between the abundance of low volatile metals in a random set of Karabash snow samples (C) and the calculated volatility of the same pure metals at the temperature of blister copper formation (12600 C). Vertical points correspond to the selected samples K(A)j the data for Si, Cu, and Fe are not considered. Figure 3. An example of correlation between the abundance of low volatile metals in a random set of Karabash snow samples (C) and the calculated volatility of the same pure metals at the temperature of blister copper formation (12600 C). Vertical points correspond to the selected samples K(A)j the data for Si, Cu, and Fe are not considered.
When the data for vanadium, nickel, cobalt, copper, and iron in petroleum of the Western Interior Region (15) shown below are divided by the average crustal abundance of these elements, the relation, V>Ni>Co>Cu>Fe is... [Pg.224]

In-vitro approach Data are available in abundance concerning metal effects on isolated chloroplasts (for a review, see Clijsters and Van Assche, 1985). All the metals studied were found to be potential inhibitors of photosystem 2 (PS 2) photosystem 1 (PS 1) was reported to be less sensitive. From the in-vitro experiments, at least two potential metal-sensitive sites can be derived in the photosynthetic electron transport chain the water-splitting enzyme at the oxidising side of PS 2, and the NADPH-oxido-reductase (an enzyme with functional SH-groups) at the reducing side of PS 1 (Clijsters and Van Assche, 1985). Moreover, in vitro, non cyclic photophosphorylation was very sensitive to lead (Hampp et al., 1973 b) and mercury (Honeycutt and Korgmann, 1972). Both cyclic and non-cyclic photophosphorylation were proven to be inhibited by excess of copper (Uribe and Stark, 1982) and cadmium (Lucero et al, 1976). [Pg.156]

FIGURE 25 Partial pressure of formaldehyde as a function of the subsurface oxygen peak area for the spectra in Figure 22A (open circles), and for a different experiment (black squares) in which the temperature of a copper foil was varied in the range from 420 to 720 K at a constant CH30H 02 molar ratio of 3 1 (the total pressure was the same as for the spectra in Fig 22A. The partial pressure of formaldehyde is linearly correlated with the abundance of subsurface oxygen in the near-surface region. The dashed line is a linear fit of the data points. [Pg.255]

The concentration intervals Ii through I5 for each element were chosen by inspecting the range of abundances using all 1027 analyses of native copper. By using the data shown in Table I, the intervals were chosen to distribute the concentrations as evenly as possible throughout the five I cells. Because many concentrations were below the detection limit, the lowest concentration interval (which includes not detected )... [Pg.277]

To illustrate the range of trace element abundances throughout the intervals through I5 for all native copper in the data base, Table I combines the 586 analyses of native copper samples from deposits throughout the world with the 441 analyses of native copper artifacts from North America. [Pg.278]

If you know the abundance of each isotope, you can calculate the average atomic mass of an element. For example, the average atomic mass of native copper is a weighted average of the atomic masses of two isotopes, shown in Figure 5. The following sample problem shows how this calculation is made from data for the abundance of each of native copper s isotopes. [Pg.253]

First of all, the data in the table are fudged for the actual irradiation space named (epithermal and fast neutron activation is included). Second, normal isotopic abundances are already factored into the tables. Let s calculate activity produced by irradiation of 2.5 grams of copper for 30 minutes. The table shows two copper activation products, Cu " and Cu . Cu " has a 4.61E4 sec (12.82 hour)... [Pg.130]


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See also in sourсe #XX -- [ Pg.301 , Pg.460 ]




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Abundance data

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