The formation of thin current sheets in the Earths magnetotail, a hallmark of the substorm growth phase, has been observed at varying radial distances...

This study aims to determine how the dayside equatorial electrojet (EEJ) is affected by substorms. There has been an ongoing debate among researchers ...

Meso-scale enhanced flow channels often extend across the polar cap from the dayside to the nightside auroral oval, where they lead to localized recon...

Winds in the nighttime upper thermosphere are often observed to mimic the ionospheric plasma convection at polar latitudes, and whether the same is tr...

The May 2024 superstorm was the most intense geomagnetic storm in more than two decades. The external driving of this superstorm consisted of a series...

It is usually thought that the strongest thermospheric winds are inside the polar cap during geomagnetic storms driven by high ion drift from cross po...

Dipolarizing flux bundles (DFBs), aka flow bursts or plasma bubbles, are transient flow structures in the magnetotail characterized by a strong northw...

It is established that flow channels associated with auroral streamers lead to substorm onset by triggering near-Earth instability. Recent studies hav...