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New Sun Images May Explain Corona's Extreme Heat

The most detailed images ever captured of the Sun's surface may help explain why its outer atmosphere, the corona, is millions of degrees hotter than its surface.

  • New images from the Inouye solar telescope show features smaller than 20km across on the Sun's surface.
  • These images reveal swirling vortices, identified as Kelvin-Helmholtz instabilities (KHIs), on the Sun.
  • Scientists believe these KHIs could explain the braiding of magnetic field lines, which may heat the corona.

Unprecedented images of the Sun's turbulent surface, captured by the Inouye solar telescope in Hawaii, show golden bands and swirling vortices. These are the most detailed pictures ever taken of our star, revealing new features smaller than 20km (12 miles) across in a magnetically active region near a sunspot.

Astronomers observed these small whirlpool-like structures, identified as Kelvin-Helmholtz instabilities (KHIs). These instabilities form when fast-moving plasma interacts with slower fluid, creating shear that leads to spiralling vortices.

Scientists suggest these processes on the surface are likely to explain the long-standing mystery of why the Sun's corona, its outer atmosphere, is millions of degrees hotter than its surface, while the surface itself is around 6,000C. Dr. David Kuridze, an astronomer on the team, stated this could solve a major mystery in solar physics.

Why this matters: Understanding the Sun's magnetic fields and explosive events, such as solar flares and coronal mass ejections, is important as these can disrupt power grids, satellites, GPS, and global communications on Earth.

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