Sentence examples for uniformly straight from inspiring English sources

Physics has Newton's first law ("Every body persists in its state of being at rest or of moving uniformly straight forward, except insofar as it is compelled to change its state by force impressed").

But if you were to put Mrs. Obama's image that day next to those of the other leaders' wives, whose clothes were uniformly straight in line, you would see someone who looked contemporary and inviting — not a drab cardboard cutout.

On other hand, the main disadvantage is that the obtained nanotubes from this technique are not necessarily uniformly straight but instead do contain some branching.

But the main drawback of LA is that the obtained CNT is not uniformly straight but instead does contain some branching.

Only the first of the three laws Newton gives in the Principia corresponds to any of these principles, and even the statement of it is distinctly different: Every body perseveres in its state of being at rest or of moving uniformly straight forward except insofar as it is compelled to change its state by forces impressed.

In particular, some or all lanes on the image are not uniformly straight, e.g., outward curving lanes, inward curving lanes and slanted lanes.

In particular, a simple one-point quadrature formula, which is typically used for quadrilateral grids, is shown to be exact for quadratic fluxes on triangular grids with uniformly spaced straight boundaries.

With the methods of Apollonius and a few infinitesimals, an inspired geometer showed that the laws regarding both area and ellipse can be derived from the suppositions that bodies free from all forces either rest or travel uniformly in straight lines and that each planet constantly falls toward the Sun with an acceleration that depends only on the distance between their centres.

The CNT was modeled as a cylinder with a length of L and a diameter of D. For the ideal state of uniformly dispersed straight CNTs in Figure 2, the simulations were carried out using a procedure to identify those CNTs being in contact, until the CNT loading reaches the required volume fraction of the CNTs in the 3D unit cell to form a global conductive network [11].

Assuming the absence of external forces, it follows (from Corollary IV to the laws) that the center of gravity of the solar system is either at rest or moves uniformly in a straight line.

In effect, we are accounting for the trajectory of the falling particle by "decomposing" it into two parts, the part determined by its natural tendency to move uniformly in a straight line, and the part contributed by the gravitational field.