Sentence examples for resolve differential from inspiring English sources

Scale modifications (as necessary to fully meet all the assumptions of the Rasch measurement model) included formation of sub-tests to deal with local response dependency (all scales except SIQTR-5 and SITB-11I), item splitting to resolve differential item functioning (all scales), and the deletion of one misfitting item (bitten fingernails to cause bleeding or pain) in the SHIF-16.

Some minor modifications to the six DSH scales were required to fully meet the assumptions of the Rasch model, namely, the formation of sub-tests to deal with local response dependency (all scales except SIQTR and SITBI), item splitting to resolve differential item functioning (all scales), and item deletion to deal with one grossly misfitting item (nail biting to cause bleeding or pain) in SHIF.

Mathematical model resolved differential equations of chest and lung movements in order to match with a clinical data base.

Figure 4 CuO NWs' intensity time-resolved differential absorption with 3.1-eV excitation (400 nm) and 770-nm probing.

Figure 3 Time-resolved differential absorption of In2O3nanocrystals excited with 325 nm and probe at 350 nm at different fluences.

In opposite to the Continuous Wave photoexcitation, we used Pulse Width Modulation of photoexcitation intensity, and confirm such behavior with a simple, time – resolved differential rate equations based model.

To further investigate the dynamics near the transition point between state filling and free carrier absorption time-resolved differential absorption measurements at various fluences were taken with probing photon energy near that region.

In order to gain a better understanding of the optical properties, time-resolved differential absorption measurements were carried out using excitation at 266 nm and probing wavelengths between 340 to 850 nm.

Figure 4 Time-resolved differential absorption of SnO2nanowires excited with 4.00 eV photons (310 nm) at fluence of 500 μJ/cm2and probe at different photon energies ranging from UV to near IR.

A typical distribution of CuO NWs obtained in this way on Si 001) is shown as an inset in Figure 2. Figure 2 CuO NWs' time-resolved differential absorption with 3.1-eV (≡400 nm) excitation and different wavelength probing.

Figure 4shows typical time resolved differential absorption measurements for the SnO2NWs excited at fluence of approximately 0.5 mJ/cm2with UV ultrafast pulses at 4.00 eV (310 nm) and probed at different photon probing energies ranging from UV to near IR.