Updated
Updated · Space.com · Aug 10
International Team Captures Sharpest Sun Image, Revealing 1st Direct Kelvin-Helmholtz Instability
Updated
Updated · Space.com · Aug 10

International Team Captures Sharpest Sun Image, Revealing 1st Direct Kelvin-Helmholtz Instability

3 articles · Updated · Space.com · Aug 10

Summary

  • Using the NSF's Inouye Solar Telescope, researchers obtained the highest-resolution image yet of the sun's surface and identified swirling structures in the solar photosphere.
  • Those swirls at the edges of magnetic regions were identified as Kelvin-Helmholtz instability — a fluid-shear effect long suspected on the sun but not directly observed there before.
  • The team said the finding exposes inner plasma dynamics that drive solar and stellar activity, with numerical simulations supporting the interpretation.
  • A Nature paper reports the work by scientists from the National Solar Observatory, NSF NCR High Altitude Observatory and Germany's Max Planck Institute for Solar System Research.

Insights

How do these newly discovered plasma swirls explain the impossible mystery of the Sun's atmosphere being hotter than its surface?
Could the tiny, swirling vortices on the Sun's surface hold the ultimate secret to predicting catastrophic space weather events on Earth?
What hidden, even smaller chaotic structures might be lurking just beyond the edge of our sharpest solar telescope's vision?