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The rock magnetic study, conducted at a core depth from 110 to 153 m below the sea floor, highlighted the widespread occurrence of magnetic iron sulfides, particularly greigite.
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The log parameters for each static Young's modulus measured in the laboratory were obtained at the corresponding core depth after adjusting the depth between the log and core data (depth shifting).
At Site C0004, the megasplay fault was recovered at 271 m CSF (core depth below the seafloor).
Finally, we classified as truly indigenous to the Tumbiana subsurface, sequences found in general at several core depths or retrieved from independent clone libraries.
We selected four samples for FORC measurements: At 0.59 and 6.91 m core depth, the two samples represented the locations where a higher peak value and a relatively constant value were recorded in the χ ARM/χ and χ ARM/SIRM ratios, respectively (Fig. 3a, b).
At 21.21 and 21.81 m core depth, the two samples were selected because of two maximum values (>0.5) presented in the χ ARM/SIRM ratio (Fig. 3b), possibly denoting the presence of magnetosomes.
The red track 1 in Fig. 8c corresponds to a correlation coefficient crossing the zero-line in signed value at about two thirds of the core depth towards the ICB (recall that it is the modulus of the correlation that is represented in this figure), meaning that the large-scale zonal flow in the lowermost part of the core is anti-correlated with its counterpart in the upper part of the core.
c f The FORC diagrams of the studied samples which obtained at 0.59, 6.97, 21.21, and 21.81 m core depth.
V p, V s, and V p/V s values at in situ condition at each coring depth were estimated assuming hydrostatic conditions (Figure 8, Table 2).
There was a strong atmospheric CO2 concentration × depth interaction effect (P C O 2 × depth = 0.009, Table 2) where elevated atmospheric CO2 levels reduced fine root N concentrations at the 10 20, 20 30 and 50 60 cm core depths, but not in the 0 10 and 80 90 cm core depths (Fig. 7).
The adiabatic gradient of the molten core can be expressed as follows (Anderson 1998): {left(frac{partial ln T}{partial ln rho}right)}_s={gamma}_{mathrm{th}} where T is a temperature at a certain depth in the outer core, ρ is the density of the core at that depth, and γ th is the thermodynamic Grüneisen parameter.
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