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The global maximum is located at the true values of the ToA and the PLE.
Its secondary maximum is located symmetrically at 20° to 50° and centered at approximately 30° of each hemisphere in eCMAM30.
A nighttime maximum is located at about 160 km and is as high as 4 · 104 cm−3.
The maximum is located between 0° and 30° S in both data and at 105 km in eCMAM30 and 105 to 110 km in SABER.
During equinox, the global distribution is marked by two dominant peaks centred at midlatitudes, while an additional weak maximum is located at very low southern latitudes.
The maximum is located at between 5° N and 20° S between September and March and at 5° S to 20° N between April and August.
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Maximum are located near the coastal areas and in the wave fronts, as expected.
For all four studied orbital positions the magnetic field maximum was located on the anti-Saturn side of Titan.
Comparison of the Fourier and HRF+TD results shows that the Fourier global maximum was located at the posterior edge of the main canonical activation.
The Fourier set global maximum was located in the posterior part of the left temporal lobe, with additional clusters in the left frontal, right anterior temporal mid-frontal, and occipital lobes.
The resulting local maximum was located in left caudal ITG (−50, −72, −12, T-score 3.78) with a nonsignificant trend in the symmetric region (40, −69, −10, T-score 2.72).
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