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In a first step, the evolution of the emissions with time is simulated on the basis of lifetime hypotheses for the technical solutions.
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The time evolution of the emission measure derived from the Bragg Crystal Spectrometer (Fe xxv channel) and from the Soft X-ray Telescope images for 27 limb flares well-observed by Yohkoh has been compared.
The evolution of the emission as a function of time is shown on Figure5a.
The data are designed to assist in understanding the evolution of these emissions on a country, regional and worldwide basis.
The distance between two QDs in the dimer QDs is estimated to be about 2 nm to 4 nm, which is due to the local thickness variation of functionalized coatings on the QDs [ 35]. Figure 4 displays typical time evolutions of the emission spectrum of a single QD, a dimeric cluster, and a trimeric cluster.
Finally, the temporal evolution of the fumarole emissions of H2O CO2 (Supplementary Fig. 1b) can be used to confine the total amount of fluid injected in each of the 14 IMF events (Supplementary Table 1) using a trial-and-error method.
The differences in the size of the flame kernel and the evolution of the radical emissions were analyzed for mixtures that fired or misfired.
Figure 8 Space-time evolution of the acoustic emissions compared to the front advance.
We discuss the temporal evolution of X-ray sources together with the evolution of the radio emission sites observed at different coronal heights by the NRH.
The evolution of the spontaneous emission, vibrational, and structural properties of MAPbI3 MWs was observed for several weeks.
Fig. 4 a PL spectra on the Si-Ge nanolayers (composition: 2(Si)/1(Ge)) in the (100) direction measured under the 488-nm excitation by using PL Systems at 17 K, in which the intensity of emission peak near 1150 nm super-linearly increases with pumping power; as shown in the inset, the evolution curve of the emission intensity at 1154 nm is increasing with pumping power super-linearly.
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