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The surface morphology and true composition of the oxide layers were investigated using SEM and EDS techniques, respectively.
The interpretations by the ROs were compared to the likelihood ratios (LRs) obtained from a probabilistic model that allows a calculation of LRs to assist the interpretation of LT DNA evidence and both were compared to the true composition of the designed mixtures.
[27] The true composition of ferric hydroxide is uncertain and variable depending upon its crystallinity with proposed examples such as Fe5HO8·4H2O (ref. [28]), Fe5(O4H3)3 (ref. [29]), 5Fe2O3·9H2O (ref. [27]), Fe4(O,OH,H2O)12 (ref. [30]) and VIFe2.9IV (Si,Fe,Al)1.3-(O,OH,H2O)12 (ref. [8]).
It is probable, however, that the true composition of ferrosic hydroxide at Franklin Seamount is closer to that of the Cl-bearing than the SO4- or CO3-bearing varieties of green rusts because the former is in much higher concentration in seawater than the latter.
Polls also likely missed the true composition of the electorate, probably including too many Democratic-leaning voters who chose to stay home.
Hence, one cannot take for granted that nifH amplicons always reflect true composition of nifH genes in situ.
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And then the approach to determine the true compositions including ionic components was given and the modified method to calculate the component fugacity of aqueous phase was developed by introducing Debye–Huckel electrostatic contribution term.
In order to improve the predicting ability of hydrate formation condition for sour gas contained systems, the dissolution of gas in water and hydrolytic reaction equilibrium existing in aqueous phase was taken into account and two concepts, i.e., the true compositions and apparent compositions of aqueous phase, were introduced.
It was beneath the trees of the grounds belonging to our house, or on the bleak sides of the woodless mountains near, that my true compositions, the airy flights of my imagination, were born and fostered".
Using this methodology, the solution of a specific problem can certainly be achieved, but attainment of the true optimal composition is never guaranteed.
It is suspected that ongoing space weathering alters the surface of the asteroids up to a few (upmu hbox {m}) depth, which modifies the optical and infrared spectra, whereas the XRF probes more than (20,upmu hbox {m}) below the surface and can reveal the true, unweathered, composition (Binzel et al. 2010).
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