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Solar Orbiter traces superfast electrons back to sun

Solar Orbiter observed over 300 bursts of solar energetic electrons, distinguishing those from flares and coronal mass ejections, enhancing space weather forecasting capabilities.

  • The ESA and NASA Solar Orbiter mission launched in 2020 traced over 300 bursts of high-energy electrons back to two distinct solar sources.
  • Scientists conducted this research to resolve why energetic electrons from solar flares or coronal mass ejections are often detected with a lag time after the events.
  • The mission found impulsive electrons originate in bursts from solar flares, while gradual electrons come from larger, longer CME eruptions, and turbulence scatters electrons delaying detection.
  • Lead researcher Alexander Warmuth stated, “We see a clear split between impulsive particle events and gradual ones associated with more extended CMEs,” highlighting the unique observations Solar Orbiter enabled.
  • This detailed understanding of solar energetic electrons will improve space weather predictions, helping protect astronauts, satellites, and spacecraft from harmful solar particle radiation.
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Phys.org broke the news in United Kingdom on Monday, September 1, 2025.
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