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NASA’s BioSentinel studies solar radiation as Earth watches aurora

In May 2024, a geomagnetic storm hit Earth, sending auroras across the planet’s skies in a once-in-a-generation light display. These dazzling sights are possible because of the interaction of coronal mass ejections—explosions of plasma and magnetic field from the sun—with Earth’s magnetic field, which protects us from the radiation the sun spits out during turbulent storms.

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