Research news on magnetic storms

Magnetic storms, more precisely geomagnetic storms, are global disturbances in Earth’s magnetosphere driven by enhanced solar wind conditions and interplanetary magnetic field (IMF) structures, particularly southward IMF associated with coronal mass ejections or high-speed solar wind streams. They are characterized by rapid energy transfer from the solar wind into the magnetosphere–ionosphere system via magnetic reconnection, causing enhanced ring current, auroral electrojets, and large deviations in geomagnetic indices such as Dst and Kp. These storms modify radiation belt populations, ionospheric currents, and thermospheric density, impacting space weather–relevant processes, including satellite drag, communications, and geomagnetically induced currents.

How the solar wind really works

The sun, our nearest star, never stops breathing. Every second of every day, it exhales a vast stream of charged particles that sweeps outward through the solar system at hundreds of kilometers per second. We call it the ...

NASA's Van Allen Probe A to re-enter atmosphere

NASA's Van Allen Probe A is expected to reenter Earth's atmosphere almost 14 years after launch. From 2012 to 2019, the spacecraft and its twin, Van Allen Probe B, flew through the Van Allen belts, rings of charged particles ...

Radio wave bursts linked to onset of intense auroral storms

A University of Southampton study has revealed an intriguing new clue in the mystery of what triggers periods of very intense, brightly colored activity during displays of both the southern and northern lights.