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Adaptive Optics Reveal Unprecedented Detail in Sun’s Corona

This breakthrough promises to deepen understanding of how coronal mass ejections and solar flares originate.

New optics show coronal rain and strange plasma features in the sun’s outer atmosphere
still from clip of corona particles falling
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Overview

  • The Cona adaptive optics system at the Goode Solar Telescope enabled the 1.6-metre mirror to achieve its 63-kilometre resolution limit, producing the sharpest images of the corona yet.
  • Colour-coded hydrogen-alpha images expose coronal rain filaments as narrow as 20 kilometres and a high-speed plasmoid jet moving at nearly 100 km/s.
  • Published May 27 in Nature, the observations bypass Earth’s atmospheric turbulence to resolve structures under 40 miles across for the first time.
  • Researchers say the detailed views of plasma loops, prominences and rain will help unveil the mechanisms driving solar storms and space weather.
  • Teams from NJIT’s Centre for Solar-Terrestrial Research and the US National Solar Observatory plan to adapt the coronal adaptive optics for larger telescopes like the Daniel K. Inouye Solar Telescope.