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In contrast, a Q–Q plot of the Fisher's exact test results (Fig. 3a) shows a large slope (slope = 2.481) and observed maximum value,, around 600 suggesting that the simple binomial model does not provide a good fit to the data.
A maximum value around 0.5 (≈ 35 at.% of N incorporation) for nitrogen rich plasmas.
This shift exhibits a maximum value around 31 wt% of VA in PVB.
The graph shows that Seebeck coefficient increases with temperature, attains a maximum value around 400 K, and decreases.
On the PSF image (Fig. 1b), the spheres had higher measured activity concentration, but the relation between the measured activity concentration and the size of a sphere was non-monotonic with a maximum value around 8 mm.
Absorption measurements have not yet been performed on such samples but photoluminescence measurements at 4 K for the same SL grown by MBE show a maximum value around 1.42 eV, in good agreement with the simulated absorption thresholds (Figure5).
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It also shows in detail that the separation of the maximum values around is 195 kHz. Figure 3 The cost function.
Conductivities showed maximum values around EC/ether mixing volume ratio = 1/1 and at about 1 M solute.
Intersection similarity values are increased with an increase in k value, with a maximum values around 0.6.
The values of the speckle cross-correlation coefficient are very low for all the data, even if not null (with maximum values around 0.01), and show different behaviours, depending on polarization.
It can be seen: (1) Hm is greater during the daytime period (06 to 18 UT) than during the night-time period (19 to 05 UT) reaching, generally, maximum values around noon (10 to 12 UT) for both solar-activity levels, HSA and LSA.
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