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The performance cycle condition is the same as for Figure 3.
Top for normal solar cycle condition, and bottom for ELSE condition.
Under the ELSE condition, the extrapolated TEC shows different latitudinal variations from those under the normal solar cycle condition.
The temperature cycle condition is −45 °C to 85 °C and the dwell time is 20 min.
Under the normal solar cycle condition, TEC peaks at the dip equator during equinoxes and at a low-latitude band of the summer hemisphere during solstices.
Under the normal solar cycle condition, the latitudinal difference of TEC's attenuation since the late afternoon is not as prominent as that under the ELSE condition.In Figure 8, TEC's seasonal variations at different latitudes were investigated with the cubic fitted TEC for the normal solar cycle condition and with the extrapolated TEC for the ELSE condition.
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Then f satisfies Axiom A and the no-cycle condition.
We prove that C 1 -generically, continuum-wise expansive diffeomorphisms satisfy both Axiom A and the no-cycle condition.
The author defines the co-cycle condition for the penalty function and shows its equivalence to strong time consistency.
Then, it is well known that Ω ( f ) = R ( f ) if and only if f satisfies the no-cycle condition.
Note that if f satisfies Axiom A and the no-cycle condition, then Ω ( f ) = R ( f ).
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