Research news on geomagnetic storm

A geomagnetic storm is a large-scale disturbance of Earth’s magnetosphere caused by enhanced coupling between the solar wind and the geomagnetic field, typically following coronal mass ejections or high-speed solar wind streams from coronal holes. It is characterized by intensified magnetospheric convection, ring current enhancement, and reconfiguration of current systems such as the auroral electrojets. Storm development and recovery phases are quantified by indices like Dst and Kp, reflecting global magnetic field perturbations. Geomagnetic storms drive strong ionospheric currents, modify radiation belt populations, enhance auroral activity, and can induce geomagnetically induced currents in conductive technological infrastructures.

How the 2024 solar superstorm drained Earth's radiation belt

In May 2024, Earth experienced its most intense geomagnetic storm since the Halloween storms of 2003. This "superstorm" filled night skies in many parts of the world with colorful aurorae, and it disrupted some infrastructure, ...

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