↳ ↑ What is a Geomagnetic Disturbance?

This page is part of the project "Understanding HF Propagation."
by Doron Tal, 4X4XM

A geomagnetic disturbance occurs when the Earth’s magnetosphere is disrupted due to interactions with solar wind, leading to changes in magnetic field strength and plasma flow.

Geomagnetic Storm Dynamics

Figure 1: Geomagnetic Disturbance based on Kakioka Magnetic Observatory, Japan
This is a typical morphology of sudden-commencement type magnetic storms (horizontal force variation).

Solar Wind
Figure 2: The solar wind interacts with Earth’s magnetosphere causing auroras.

When a CME enters the magnetosphere, it causes a Geomagnetic Storm

Figure 3: Interaction between a CME and Earth's Magnetosphere

A major magnetic storm may block HF propagation (3–30 MHz) by modifying the distribution of free-electrons in the ionosphere.


The project "Understanding HF Propagation," focuses on skywave propagation,
shows near-real-time indices and explains what the terms mean.

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