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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.
These values are comparable to the NADPH production rates that also reach maximum values around 0.02 pmol/pl/h.
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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.
The Doppler shift of this trace became increasingly more negative during the PSSR of the F layer, and reached a maximum value around 1830 UT (indicated by a downward-pointing red arrow), which is close to E-region sunset (SS E ).
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