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A secondary maximum clearly appears in X at mid-latitudes.
It is particularly strong in X, which also displays a secondary maximum towards the geomagnetic equator.
There is a secondary maximum located at 10° to 20° S and 100 km.
The secondary maximum amplitude is mainly 3 to 5 K for both eCMAM30 and SABER.
Its secondary maximum is located symmetrically at 20° to 50° and centered at approximately 30° of each hemisphere in eCMAM30.
Turbulence characteristics of a relatively "quiet" downstream decreasing internal wake region, located well below the secondary maximum points of the mean velocity distributions, are described.
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However, its primary and secondary maxima are reversed from their counterparts at 45 km.
Most SPW modes have secondary maxima at altitudes 80 100 km in the northern hemisphere.
These secondary maxima were attributed to the fluorescence of protein-like substances [25, 26].
The secondary maxima at the mid- and high latitudes seen at 95 km are absent at this altitude in eCMAM30.
The F0.5 layer has a June (northern summer) solsticial maximum probability of occurrence with secondary maxima during December (northern winter) solstice.
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