This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: 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.
Coronal mass ejections (CMEs) are giant expulsions of magnetized plasma from a star's atmosphere into space. They play a major role in shaping stellar evolution, driving mass and angular momentum loss, and influencing the space weather environments of orbiting planets. While they are routinely observed on the sun, convincing detections around other stars have remained surprisingly scarce.
The study, published in Physical Review Letters, combines astrophysical simulations, high-energy laser-plasma experiments and advanced three-dimensional numerical plasma modeling. The results show that strong magnetic fields of active stars can completely suppress CMEs before they escape into space. "The unique combination of theory, laboratory tests, and numerical simulations provides the first experimental evidence supporting a long-standing prediction that stellar magnetic fields can confine these large-scale eruptions," said Julián D.
Alvarado-Gomez, senior scientist in the Stellar Physics and Exoplanets research group at the Leibniz Institute for Astrophysics Potsdam (AIP). He contributed the astrophysical modeling that connects the laboratory experiments to real stellar environments. Using scaling laws that faithfully reproduce astrophysical conditions, the international team generated laser-driven plasma flows in the laboratory to mimic the core of stellar CMEs.
When exposed to relatively weak ambient magnetic fields, the plasma propagated freely. However, stronger magnetic fields caused the flow to fragment, become unstable and ultimately stop altogether. "This actually came as a surprise when we were increasing the magnetic field strength and observed the change in behavior of the propagating plasma, but this is the essence of experimental discovery," said Julien Fuchs, then senior scientist at LULI/CNRS in France and now professor at Technion in Israel.
Detailed numerical plasma simulations identified a kink instability as the physical mechanism responsible for disrupting the eruption. In the laboratory experiment, the eruption was triggered by the laser striking the target, which increased the target's thermal pressure and caused the plasmoid to expand and move. The kink instability occurred in the plasma flow when the external magnetic field was strong enough, causing the flow to bend and even travel backward.
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