Sentence examples for disk surface of from inspiring English sources

Composite film electrodes containing mechanically mixed MnxCu1−xCo2O4 (0 ≤ x ≤ 1) particles, carbon black Vulcan XC72R and poly vinylidene fluoride-co-hexafluoropropylene) (PVdF-HFP) were formed on the glassy carbon disk surface of a rotating ring-disk electrode (RRDE) and studied for the oxygen reduction and evolution reactions (ORR and OER, respectively) in 1 M KOH solution.

Due to technical challenges in the structural characterization of the nucleosome core bound to chromatin factors, much less is understood regarding the molecular recognition of the disk surfaces of the histone octamer and nucleosomal DNA.

The impact of disk surface features and the positions of the trailing pad, the side pads, the leading pads and the negative pressure center on FHM are also investigated using parametric analysis.

The relaxation processes was found to progress in this material as a result of the gradual heating of disk surface.

It was also found that at a designed groove depth of 4 8 nm, the shallow FIB etched grooves already provide good isolation between adjacent tracks, indicating the importance of ion beam induced modification of magnetic properties in film media over physical modification of disk surface topography.

Today, a more refined version of the writing and reading heads that descended from Dr. Bajorek's research "fly" over the disk surface at a height of about 150 angstroms (an angstrom is roughly the width of a single hydrogen atom).

The amount of data that can be squirrelled away on a square inch of disk surface (the industry clings obstinately to imperial measurements) has increased by 60% every year since 1991.

The discrepancy in the temperatures comes mainly from the different choice of the height of the disk surface at which the disk receives the radiation from the central star.

The analysis results show that the improvement of the roll-off characteristics of the disk surface waviness can also decrease the FHM.

Note that the height of the disk surface is determined by a balance between the dynamical pressure of the wind and the gas pressure in the disk which is proportional to the local matter density.

The heights of the disk surface are shown in Fig. 3(a) for five cases of t*/ β from 1 × 108 yr to 1 × 1012 yr.