Tue. Nov 5th, 2024
Occasional Digest - a story for you

Flares and coronal ejections shooting off from the Sun’s surface struck the Earth overnight, causing a severe geomagnetic storm.

It was the strongest such event in about 20 years, leading to stunning aurora australis light displays in skies across southern parts of Australia and the southern hemisphere.

People in the northern hemisphere also saw and photographed stunning images of pink, red, green and violet skies brought on by the aurora borealis early on Saturday morning.

The solar event is predicted to continue over the weekend, bringing more bright aurora light shows with it.

But what are geomagnetic storms exactly, and how do they produce auroras?

What is a geomagnetic storm?

Geomagnetic storms originate from a specific type of activity taking place on the Sun.

Large “clouds” containing billions of tonnes of plasma embedded within an ejected magnetic field erupt from the Sun’s outer atmosphere, or corona.

These eruptions are known as coronal mass ejections (CMEs).

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Unlike solar flares, which travel at the speed of light and reach Earth in about eight minutes, CMEs travel at a more sedate pace.

Officials put the current average at 800 kilometres per second.

These ejections sometimes travel towards Earth, where they can temporarily disturb the Earth’s magnetosphere, resulting in geomagnetic storms.

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