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Parker Solar Probe reveals why the sun’s corona is weirdly hot

As Parker Solar Probe files around the sun, it finds abrupt reversals in the direction of the sun’s magnetic fields. These S-shaped bends in the sun’s magnetic field are very common in the solar wind close to the sun, but are absent inside the corona.

The sun's crown-like atmosphere can be 200 times hotter than the sun's surface.

Continue reading Parker Solar Probe reveals why the sun’s corona is weirdly hot on Tech Explorist.


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