The maximum power density tends to increase with increasing pressure while the micro-channel length and height associated with the maximum tend to decrease.
Several possible values of K were indicated by this method but the maxima tended to be less reliable between runs at higher K values.
In addition, the nighttime maximum tends to occur at earlier local time.
The magnitude of the two mid-latitude maxima is similar in eCMAM30, while the NH mid-latitude maximum tends to be stronger than the SH counterpart in SABER.
(11) From (10) together with (11) it follows that (Lambda_{n} (E )) and (m_{n} (E ) ) are of different orders of magnitude, and hence the maximum deviation (delta _{n} ({E} )) of the local maxima tends to infinity exponentially fast.
The 1.5-LOD support interval, meaning the interval in which the LOD score was within 1.5 units of its maximum, tended to be smaller in the high-density map (average of 14.62 ± 18.03 cM) than in the SSR map (22.01 ± 19.85 cM), but the difference was not significant (P = 0.129) (Table 4).
Both of them reach the maximum and tend to be stable when θ is greater than 0.5.
Theoretically, GAD tends to the maximum displacement when n tends to infinity (Li and Fang 1997), i.e., U GAD → n → ∞ max u x, x ∈ Ω Open image in new window.
It can be seen that the day of the maximum amplitude of tends to appear 7 days after the local summer solstice (i.e., June 21 for Kakioka and December 21 for Gnangara).
The maximum local density tends to reach a plateau at 4 5 mg L-1, which is an estimate of the upper limit of density tolerance under the given food conditions.
