Investigation of the post-sunset extra electron density peak poleward of the Equatorial Ionization Anomaly southern crest

This Ne peak is different from previously reported mid-latitude peaks that occur at all local times. The Whole Atmosphere Community Climate Model-eXtended captures this phenomenon.

Model diagnostic analysis reveals that the decrease of Ne and hmF2 between 15 degrees and 25 degrees S makes Ne near 30 degrees S appear as an extra density peak relative to the southern EIA crest. Transport by poleward meridional wind decreases Ne between 15 degrees and 25 degrees S. Moreover, the upward E x B drifts due to pre-reversal enhancement lift the plasma between the dip equator and 15 degrees S but do not affect Ne much between 15 degrees and 25 degrees S with a low drift speed.