Spaceweather Glossary

Learning aurora terminology

← Back to Map

Glossary of Common Terms

Aurora
Colorful lights in the sky caused by charged solar particles hitting Earth’s atmosphere, commonly seen near the poles.
Kp Index
A global scale (0–9) that estimates geomagnetic activity. Kp 5 or higher is often aurora-worthy.
Bz
The north-south direction of the interplanetary magnetic field. A negative (southward) Bz allows aurora to form more easily.
Solar Wind
A stream of charged particles from the Sun that fuels auroras when it interacts with Earth’s magnetosphere.
Coronal Hole
An opening in the Sun’s atmosphere that releases high-speed solar wind, often triggering geomagnetic storms.
Geomagnetic Storm
A disturbance in Earth’s magnetic field caused by solar wind, which can enhance aurora activity.
Hemispheric Power
A NOAA estimate of how much power is going into auroral activity in gigawatts (GW). Higher = more visible aurora.
IMF
Interplanetary Magnetic Field — the magnetic field carried by the solar wind. Its direction and strength influence aurora visibility.
Bt
The total strength of the interplanetary magnetic field. Higher values often indicate stronger aurora potential when paired with southward Bz.
Share This Page