Sentence examples for the outward surface from inspiring English sources

Exact(1)

The enriched Co in the near-surface region, with consequent increase of Co atomic distribution, not only induces ligand effects but also compresses the surface Pt Pt bond distance by suppressing the outward surface relaxation.

Similar(59)

The program note suggested that the works by Mozart, Ravel and Chopin that Mr. Zimerman chose share a quality in which outward surface beauties distract the listener from the inner structures.

For simplification of the procedure, regrinding of this instrument and minimization of the nascent "organic" error at regrinding on the outward cylindrical surface, a decision was made to bring in the instrument construction developed by N.V. Smorkalov et al. of positive rake γ, form a radius ditch and two antihunt ribbons breadthways l executed on an outward cylindrical surface.

If moisture leaks through the sterile portion of a dressing to any outward surface which is not sterile, you have a culture medium extending all the way from the surface down to the wound.

All the geometrical properties of the considered surface can be derived from φ, such as the outward-pointing surface normal (hat {mathbf {n}}= - nabla varphi / | nabla varphi |).

(gamma (hat {mathbf {n}})) is the surface energy density, with (hat {mathbf {n}}) the outward-pointing surface normal, and ε the thickness of the interface between phases.

A βσ represents the area of the β σ interface; n βσ is the outward-directed surface normal from the β-phase toward the σ-phase, and n βσ = −n σβ (Fig. 7). Figure 7 Nanofluids and representative elementary volume (REV).

Another clear difference in conformation was found on the outward-facing surface of complex IV, where a helix of subunit VIb sticks out of the supercomplex density but is readily accommodated in an adjacent unoccupied, roughly equal map volume.

where n is the outward normal to the surface at r s [15].

Let ∂ ∂ n and d σ denote the outward normal derivative and surface measure, respectively, on the boundary ∂ Ω of Ω.

But for all other stars, their sizes are determined by that simple balance: the force from the outward radiation, at the surface, has to equal the inward pull of gravitation.

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