Skip to content
Home Academy Space Weather Geomagnetic Storms (G-scale)
LESSON 04 OF 6

Geomagnetic Storms (G-scale)

Beginner ~7 min Slide deck Free

When the solar wind or a CME disturbs Earth's magnetic field, we call it a geomagnetic storm. NOAA's G-scale (G1–G5) ranks the severity — and each step up brings significantly more impact to technology and infrastructure.

When the solar wind or a CME disturbs Earth's magnetic field, we call it a geomagnetic storm. NOAA's G-scale (G1–G5) ranks the severity — and each step up brings significantly more impact to technology and infrastructure.

What this lesson covers

What triggers a geomagnetic storm

A geomagnetic storm occurs when sustained energy transfer from the solar wind disturbs Earth's magnetosphere. The key inputs are solar wind speed, density, and — most critically — a sustained southward IMF (negative Bz).

Real-world impacts

Geomagnetic storms aren't just an aurora trigger — they cause measurable problems across multiple technology sectors.

Key facts

💡The Dst (Disturbance Storm Time) index measures ring current intensity. Below −50 nT = moderate storm. Below −250 nT = extreme.
G1 is common and manageable. G5 is rare and genuinely dangerous to modern infrastructure.

The G-scale gives operators a shared language to prepare. Most space weather is routine — but the tail risk from extreme events is why governments and grid operators take it seriously.

All lessons in Space Weather
01KP Index (what it actually measures)~8 min02Solar Wind (speed, density, IMF)~7 min03CMEs → Aurora (the chain reaction)~8 min04Geomagnetic Storms (G-scale)~7 min05How Space Weather Affects Satellites~8 min06Space Weather Forecasting (what's possible)~7 min
← CMEs → Aurora (the chain reaction)All 6 LessonsHow Space Weather Affects Satellites →
🪐Support Us