Sentence examples for sufficient brightness from inspiring English sources

So the company's prototypes either use a conventional, larger blue sub-pixel or rely on blue light in a white subpixel to achieve sufficient brightness.

We show that sufficient brightness and uniform signal to noise ratio (SNR) can be achieved within the indoor coverage by using the proposed optimal LED arrangement, thus enabling the terminal mobility for indoor VLC.

We have studied the radiometric and spectral characteristics of LID scatterers and found that they have the properties needed to display objects in color and with sufficient brightness to be viewed within a 120 degree cone that is aligned with the projection direction.

- having sufficient brightness and color capabilities to deliver at least some of HDR's picture quality benefits.

The sufficient brightness and photostability make QDs favorable for tracking intracellular events.

If the light could be focused in sufficient brightness, someday it might make a beam weapon.

With both methods, synchrotron light is needed to provide sufficient spectral brightness for diffraction-limited spatial resolution, although globar sources and benchtop instruments are well suited to imaging larger samples at spatial resolutions of approximately double the diffraction limit, making them a competitive alternative to synchrotron-based FTIR imaging for some samples.

A Deskey representative said "seeability" is important - this means adequate pavement brightness, sufficient object brightness, a low level of discomfort glare & a minimum of disability-veiling glare.

Parameters used in the process are obtained by the particle swarm optimization algorithm, ensuring that the output image contains sufficient contrast and brightness.

Furthermore, experience is gathered while performing these simulations, e.g. the examination of the pulse shapes obtained with time-dependent calculations shows that for long-pulse target stations the peak brightness can with sufficient precision be obtained from time-independent calculations by scaling with the proton pulse duty factor.

He joined the UC Berkeley faculty in 1982 and has emerged as a world expert in the study of "brown dwarfs," which are stars without sufficient mass to have a stable brightness and that end up cooling down to planetary temperatures.