"SolarMetrics... bringing space weather down to Earth!"

Real-Time Space Weather


Solar Flare
Solar X-rays are emitted at the onset of a solar flare. A large flare can cause loss of HF communications through ionisation of the ionosphere. Complex magnetic loop structure and bright regions indicate locations of high solar activity that are likely to release solar flares or coronal mass ejections.
Solar Particle Event
Coronal Mass Ejection
 
Geomagnetic Storm
   
Aurora
   
Ionsospheric Absorption