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Stellar eruptions in the laboratory: First experimental evidence for their suppression in strong magnetic fields

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An international team of astrophysicists and plasma physicists has provided the first experimental evidence that strong magnetic fields surrounding active stars can completely suppress coronal mass ejections. This offers clues to why massive stellar eruptions are rarely observed on stars other than the sun.

Key takeaways

  • 01An international team of astrophysicists and plasma physicists has provided the first experimental evidence that strong magnetic fields surrounding active stars can completely suppress coronal mass ejections.
  • 02This offers clues to why massive stellar eruptions are rarely observed on stars other than the sun.
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