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The separation between the maxima of the two peaks corresponding to these two viscoelastic mechanisms is obtained for several temperatures.
Second, using the GIM tensors for different UT intervals, between the maxima of ionospheric (U^{(2)}) and solar irradiation, the time lags can be obtained.
Furthermore, the time lags between the maxima of the ionospheric (U^{(2)}) and solar irradiation range from 1 to 3.7 h without seasonal dependence.
Our results provide evidence for the time lag between the maxima of large-scale ionospheric variations and solar irradiation, though we cannot provide an exact explanation for its mechanism due to observational limitations.
As shown, the longitude differences between the maxima of large-scale longitudinal variations and those of solar irradiation in (U^{(2)}) are the same as those in Fig. 3.
The energy difference between the maxima of absorption (370 nm, 3.35 eV) and emission spectra (501 nm, 2.48 eV) has been mainly attributed to trap sites within the band-gap [16].
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Participant age range was normally distributed with the majority falling between the maximum of 31 40, (20, 36.4 %); followed by those within the age range of 20 30, (18, 33 %).
The method provides results for two different linear relations, namely the relationship between thickness and slope in the 560 580 nm range and ratio between the maximum of the slope and the wavelength at that maximum slope.
If a band gap is assumed in a semiconductor with parabolic bands (see also Fig. 6), size quantization increases the energetic spacing between the maximum of the valence band and the minimum of the conduction band for the 1D case.
The schedule is composed by cycling between the maximum of L+1 involved link rate vectors until there are ⌈α k δ (L + 1)⌉ occurrences of each vector v k.
Also, due to a small offset between the maximum of the frequency in the Gain curve of the QCL and the 1912 cm 1 IR absorption band peak.
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