An X6.3 solar flare occurred on Feb 22, 2024, one of the biggest flares with a clear EUV late phase (ELP). A unique feature of ELP is that it has a se...

This study explores the feasibility of fusing satellite measurement inferred ionospheric total electron content (TEC) and traditional ground-based TEC...

The energy coupling between the solar wind and magnetosphere and the internal dynamics within the tail of the magnetosphere have both been shown to be...

Ionospheric density variation affects the propagation of radio signals, such as the Global Navigation Satellite System (GNSS) signals and over-the-hor...

Equatorial Plasma Bubbles (EPBs) are one of the most severe space weather phenomena that occur in the ionosphere causing high levels of radio scintill...

The Equatorial Plasma Bubbles (EPBs) are low-density plasma structures embedded in the large-scale Equatorial Ionization Anomaly (EIA). They are known...

We study the impact of evolving ionospheric high-density structures, e.g., storm enhanced density (SED) and SED plumes, on upward ion fluxes during th...

Accurately predicting the horizontal component of the ground magnetic field perturbation (dBH), as a proxy for Geomagnetically Induced Currents (GICs)...