Abstract
A unique phenomenon {\textendash} merging of Equatorial
Ionization Anomaly (EIA) crests, leading to an X-pattern (EIA-X) around
the magnetic equator {\textendash} has been observed in
the night-time ionospheric measurements by the Global-scale Observations
of the Limb and Disk (GOLD) mission. A whole atmospheric general
circulation model simulation reproduces this pattern. The pattern is
also produced in an assimilative ionosphere model that assimilates slant
Total Electron Content (slant-TEC) from Global Navigation Satellite
System (GNSS) and Constellation Observing System for Meteorology,
Ionosphere, and Climate 2 (COSMIC-2). Due to the observed similarity
between measurements and simulations, the latter is used to diagnose
this heretofore unexplained phenomenon. The simulation shows that the
EIA-X occurs in the afternoon to evening sector at a longitude where the
vertical drift is negative, which is a necessary but not sufficient
condition. The simulation was performed under constant low-solar and
quiescent-geomagnetic forcing conditions, therefore we suggest that one
of the drivers of this phenomenon is from lower-atmospheric processes.