The equatorial electrojet (EEJ) is an intense, narrow eastward current system flowing within the daytime ionospheric E region (~105–110 km altitude) along the magnetic dip equator. As a crucial component of low-latitude space weather, understanding the EEJ's variability is essential for protecting global communication and navigation networks. Led by researchers from Wuhan University, this newly published review presents a systematic synthesis of the spatial and temporal evolution of the EEJ. Under geophysically quiet conditions, the EEJ displays pronounced local time and longitudinal variations. Ground and satellite observations demonstrate that while solar photoionization controls its daytime peak near local noon, nonmigrating atmospheric tides originating from tropical tropospheric convection dictate its global wave-4 longitudinal structure. Beyond quiet-time climatology, the review pays critical attention to the EEJ’s behavior under highly volatile space weather conditions. It delineates how energy inputs from mid- and high-latitude regions can rapidly alter or even reverse the electrojet's direction—creating a westward counter electrojet (CEJ). These perturbations are driven by two main processes: prompt penetration electric fields (PPEF) that map instantly from high latitudes during storms, and disturbance dynamo electric fields (DDEF) driven by long-lasting storm-time thermospheric winds. Other cross-regional factors, such as magnetospheric substorms, sudden changes in solar wind dynamic pressure, subauroral polarization streams (SAPS), and sudden stratospheric warmings (SSWs), are shown to introduce stark asymmetries into low-latitude dynamics. Furthermore, the review addresses the distinct pathways of solar radiative forcing, such as solar flares and eclipses, which modulate the EEJ through rapid adjustments in ionospheric conductivity and dynamo interactions. While state-of-the-art physics-based numerical simulations (like the TIEGCM) and data-driven empirical frameworks have successfully reproduced basic seasonal and diurnal structures, their quantitative consistency remains limited during major space weather disturbances. The authors point out critical open issues, including the lack of unified frameworks for multi-factor coupling and the unmodeled nonlinear responses of the ionosphere. Resolving these bottlenecks will require the strategic integration of multi-platform coordinated observations, refined parameterizations of high-latitude boundaries, and data-driven machine learning models.
Earth and Planetary Physics
A review of the climatology features and mid- and high-latitude forcing of the equatorial electrojet
1-Jul-2026