Sentence examples for rotation surface from inspiring English sources

All retrieved bearings showed rotation surface damage, but severity of the damage did not correlate with duration.

Rotation surface damage appeared to be caused by contaminant particles, which produced curvilinear scratches that were longer than the normal rotational excursion of the knee.

Source-to-ground distances of 10, 15 and 20 cm, solids concentrations of 12 and 18 wt.% and mandrel rotation surface speeds of 0 12 m s−1 were utilized.

The RTI of two superposed incompressible fluids of different densities in the presence of small rotation, surface tension and suspended dust particles is investigated by Sharma et al. [40].

The influences of rotation and surface blowing on the streamlines, the flame-front geometry, the flame stretch, as well as the torque on rotating porous spheres are determined.

An interesting feature associated with particle rotation and surface blowing is that they can affect the near wake structure in such a way that an unsteady three-dimensional flow with vortex shedding develops at lower Reynolds numbers as compared to flow over a solid sphere in the absence of these effects, and thus, the temperature distributions around the particle are significantly affected.

There, it was pointed out that grain reorientations occur by grain boundary migration, grain rotation, and surface diffusion, which are exactly the processes that we can now observe at atomic resolution using the electron beam as a stimulus.

Astronomers will be able to study the asteroid's size, shape, rotation, and surface features -- all of which could shed light on its origin.

Theory predicts that, owing to Altair's rapid rotation, its surface gravity and effective temperature should be lower at the equator, making the equator less luminous than the poles.

For dust particles within the belt, typical temperatures range from 200 K (−73 °C) at 2.2 AU down to 165 K (−108 °C) at 3.2 AU However, due to rotation, the surface temperature of an asteroid can vary considerably as the sides are alternately exposed to solar radiation and then to the stellar background.

The equations have been used to predict the mid-span deflections, support rotations and surface strains recorded during the flexure tests.