A well-studied solar phenomenon may not be quite as simple as we we thought it was.
erupting out from the surface of the Sun along magnetic field lines may, at least sometimes, be wrinkles in corrugated sheets of plasma., and suggest that further research is needed to try to understand how and why they occur.
Firstly, coronal loops associated with sunspots tend to be much taller than calculations suggest they should be. However, the simulation also revealed that coronal loops can exist on their own, too. This suggests that the solar corona is a much more complex environment than we knew.
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