Sentence examples for maximum luminosity and from inspiring English sources

Most are spectral type F (moderately hot) at maximum luminosity and type G (cooler, Sun-like) at minimum.

Flame areas defined by the loci of maximum luminosity and by schlieren contours were recorded, so that saturation current densities, CH∗ and C∗2 emission per unit flame area, as well as burning velocities could be deduced.

A maximum luminosity of 2×1032 cm−2s−1 and an energy resolution of about 100 keV at lower luminosity are main objectives of the HESR concept.

A nova reaches maximum luminosity within hours after its outburst and may shine intensely for several days or occasionally for a few weeks, after which it slowly returns to its former level of luminosity.

energy range from 2 to 5 GeV with a maximum luminosity of 1035cm−2s−1 is designed to study physics of τ lepton, charmed hadrons and e+e− annihilation with very high precision.

In contrast, at radio wavelengths the maximum luminosity for spirals is usually 100,000 times less than for ellipticals or irregulars.

The two separate collider rings cross at six interaction points, where the lattice design provides low-beta insertions for maximum luminosity.

From the images of OH PLIF and CH chemiluminescence and the Rayleigh concentration measurement, it has been shown that the positions of maximum luminosity in direct photographs of lifted tribrachial flames can reasonably be located along the stoichiometric contour.

It exceeds the one of the ATLAS muon drift tube (MDT) chambers, which are operated at unprecedentedly high background rates of neutrons and γ-rays, by an order of magnitude, which is sufficient for almost the whole of the muon detector acceptance at FCC-hh at maximum luminosity.

This is done by using the plugin 'Temporal-Color Coder' in ImageJ which provides as a last step a merged image that shows pixel by pixel the frame number in which the maximum luminosity of the stacked frames is reached (Miura 2008).

Near the time of maximum luminosity, the spectrum contains lines of intermediate-mass elements from oxygen to calcium; these are the main constituents of the outer layers of the star.